The image is based on data from ESA's Planck satellite, which scanned the sky between 2009 and 2013 to study the cosmic microwave background [CMB], the most ancient light in the Universe's history.
While doing so, Planck also detected foreground emission from material in the Milky Way, as well as from other galaxies.
The red clumps at the centre of the image are part of the Orion Molecular Cloud Complex, one of the closest large regions of star formation, only about 1300 light-years from the Sun.
The most prominent of the red clumps, to the lower left of centre, is the famous Orion Nebula, also known as M42.
This is visible to the naked eye in the constellation Orion, just below the three stars forming the 'belt' of the mythological hunter. An annotated version of the image can be found here.
Planck's main goal was to provide the most precise map of the relic radiation of the Big Bang, the cosmic microwave background [CMB].
To do so, it surveyed the entire sky in nine different wavelengths from the far-infrared to radio, in order to eliminate foreground emission from our galaxy and others in the Universe.
High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE, is authored by the Planck Collaboration.
The European Space Agency's Planck observatory peered back into the universe's history to study the cosmic microwave background, the oldest light in the universe. See images from Planck's prolific mission in this Space.com gallery. Here: An artist's view of Planck with the cosmic microwave background as a backdrop.
A view of the Milky Way galaxy in microwaves, captured by the European Space Agency's Planck satellite. The different colors correspond to different elements, including gas, dust, and energetic particles.
This map of the Milky Way shows the distribution of interstellar dust across the galaxy as seen by the Planck space observatory, a mission by the European Space Agency. ESA and NASA unveiled the image on Feb. 5, 2015.
Each of the four bottom) show a specific subset of Planck observations that make up the combined view (top). Of the subsets, they show: Top left is dust, top right is gas, bottom right is light from charged particle interactions, and bottom right shows charged particles moving along the galaxy's magnetic field.
All of the matter between Earth and the edge of the observable universe is shown in this image based on data from the European Space Agency's Planck space observatory. This map was released on Feb. 5, 2015.
This image unveiled March 21, 2013, shows the cosmic microwave background (CMB) as observed by the European Space Agency's Planck space observatory. The CMB is a snapshot of the oldest light in our Universe, imprinted on the sky when the Universe was just 380 000 years old. It shows tiny temperature fluctuations that correspond to regions of slightly different densities, representing the seeds of all future structure: the stars and galaxies of today.
This European Space Agency graphic depicts the most refined values yet of the Universe's ingredients, based on the first all-sky map of the cosmic microwave background by the Planck space observatory unveiled on March 21, 2013. Normal matter that makes up stars and galaxies contributes 4.9 percent of the Universe's mass/energy inventory. Dark matter occupies 26.8 percent, while dark energy accounts for 68.3 percent.
Two Cosmic Microwave Background anomalies hinted at by the Planck observatory's predecessor, NASA's WMAP, are confirmed in new high-precision data revealed on March 21, 2013. In this image, the two anomalous regions have been enhanced with red and blue shading to make them more clearly visible.
This European Space Agency graphic shows a map of the universe that depicts the anomalies seen when comparing the Planck space observatory's map of the universe's cosmic microwave background and the standard model of the cosmos. Image released March 21, 2013.
his all-sky image shows the spatial distribution over the whole sky of the galactic haze at 30 and 44 GHz, extracted from the Planck observations. Image released February 13, 2012.
Credit: ESA/Planck Collaboration; T. Dame et al.
This all-sky image shows the distribution of carbon monoxide (CO), a molecule used by astronomers to trace molecular clouds across the sky, as seen by Planck (blue). A compilation of previous surveys (Dame et al. (2001)), which left large areas of the sky unobserved, has been superimposed for comparison (red). The outlines identify the portions of the sky covered by these surveys. Image released February 13, 2012.
This image shows the Cepheus molecular cloud complex as seen through the glow of carbon monoxide (CO) with Planck (blue). The same region is shown as imaged by previous CO surveys (Dame et al., 2001) for comparison (red). Image released February 13, 2012.
This all-sky image shows the distribution of carbon monoxide (CO), a molecule used by astronomers to trace molecular clouds across the sky, as seen by Planck. The inserts provide a zoomed-in view onto three individual regions on the sky where Planck has detected concentrations of CO: Cepheus, Taurus and Pegasus, respectively. Image released February 13, 2012.
All-sky Distribution of Carbon Monoxide (CO).
This all-sky image shows the distribution of carbon monoxide (CO), a molecule used by astronomers to trace molecular clouds across the sky, as seen by Planck (blue). A compilation of previous surveys (Dame et al. (2001)), which left large areas of the sky unobserved, is shown for comparison (red). Image released February 13, 2012.
This image shows the Taurus molecular cloud complex as seen through the glow of carbon monoxide (CO) with Planck (blue). The same region is shown as imaged by previous CO surveys (Dame et al., 2001) for comparison (red). Image released February 13, 2012.
This image shows molecular clouds in the Pegasus region as seen through the glow of carbon monoxide (CO) with Planck (blue). Image released February 13, 2012.
This multi-frequency all-sky image of the microwave sky has been composed using data from Planck covering the electromagnetic spectrum from 30 GHz to 857 GHz. This image was released on July 5, 2010. The mottled structure of the cosmic microwave background, with its tiny temperature fluctuations reflecting the primordial density variations from which today's cosmic structure originated, is clearly visible in the high-latitude regions of the map. The central band is the plane of our Galaxy. A large portion of the image is dominated by the diffuse emission from its gas and dust. The image was derived from data collected by Planck during its first all-sky survey and comes from observations taken between August 2009 and June 2010. This image is a low- resolution version of the full data set.
Planck's orbit around L2, the second Lagrange point of the Sun-Earth system.
The image spans about 50 degrees of the sky. It is a three-colour combination constructed from Planck's two highest frequency channels (557 and 857 GHz, corresponding to wavelengths of 540 and 350 micrometres), and an image at the shorter wavelength of 100 micrometres made by the IRAS satellite. It was released on March 17, 2010.
An active star-formation region in the Orion Nebula, as seen By Planck. This image covers a region of 13×13 degrees. It is a three-colour combination constructed from three of Planck's nine frequency channels: 30, 353 and 857 GHz. This image was released on April 26, 2010.
The microwave sky as seen by ESA's Planck satellite. Light from the main disk of the Milky Way is seen across the center band, while radiation left over from the Big Bang is visible on the outskirts of the image.
This image shows the location of the first six fields used to detect and study the Cosmic Infrared Background. The fields, named N1, AG, SP, LH2, Boötes 1 and Boötes 2, respectively, are all located at a relatively high galactic latitude, where the foreground contamination due to the Milky Way's diffuse emission is less dramatic. It was released on Jan. 11, 2011.
"But there is more: the CMB carries additional clues about our cosmic history that are encoded in its 'polarisation'," explains Jan Tauber, ESA's Planck project scientist.
"The polarisation of the CMB also shows minuscule fluctuations from one place to another across the sky: like the temperature fluctuations, these reflect the state of the cosmos at the time when light and matter parted company," says François Bouchet of the Institut d'Astrophysique de Paris, France.
"After the CMB was released, the Universe was still very different from the one we live in today, and it took a long time until the first stars were able to form," explains Marco Bersanelli of Università degli Studi di Milano, Italy.
"Planck's observations of the CMB polarisation now tell us that these 'Dark Ages' ended some 550 million years after the Big Bang – more than 100 million years later than previously thought.
This key phase in the history of the cosmos is known as the 'epoch of reionisation'.
"From our measurements of the most distant galaxies and quasars, we know that the process of reionisation was complete by the time that the Universe was about 900 million years old," says George Efstathiou of the University of Cambridge, UK.
Planck's new results are critical, because previous studies of the CMB polarisation seemed to point towards an earlier dawn of the first stars, placing the beginning of reionisation about 450 million years after the Big Bang.
This posed a problem. Very deep images of the sky from the NASA–ESA Hubble Space Telescope have provided a census of the earliest known galaxies in the Universe, which started forming perhaps 300–400 million years after the Big Bang.
"In that case, we would have needed additional, more exotic sources of energy to explain the history of reionisation," says Professor Efstathiou.
"These are only a few highlights from the scrutiny of Planck's observations of the CMB polarisation, which is revealing the sky and the Universe in a brand new way," says Jan Tauber.
"A Joint Analysis of BICEP2/Keck Array and Planck Data" by the BICEP2/Keck and Planck collaboration has been submitted to the journal Physical Review Letters.
While the pastel tones and fine texture of this image may bring to mind brush strokes on an artist's canvas, they are in fact a visualisation of data from ESA's Planck satellite. The image portrays the interaction between interstellar dust in the Milky Way and the structure of our Galaxy's magnetic field.
Interstellar clouds of gas and dust are also threaded by the Galaxy's magnetic field, and dust grains tend to align their longest axis at right angles to the direction of the field. As a result, the light emitted by dust grains is partly 'polarised' – it vibrates in a preferred direction – and, as such, could be caught by the polarisation-sensitive detectors on Planck.
Scientists in the Planck collaboration are using the polarised emission of interstellar dust to reconstruct the Galaxy's magnetic field and study its role in the build-up of structure in the Milky Way, leading to star formation.
In this image, the colour scale represents the total intensity of dust emission, revealing the structure of interstellar clouds in the Milky Way. The texture is based on measurements of the direction of the polarised light emitted by the dust, which in turn indicates the orientation of the magnetic field.
While the pastel tones and fine texture of this image may bring to mind brush strokes on an artist's canvas, they are in fact a visualisation of data from ESA's Planck satellite.
The image portrays the interaction between interstellar dust in the Milky Way and the structure of our Galaxy's magnetic field.
Our Galaxy's magnetic field is revealed in a new image from ESA's Planck satellite. This image was compiled from the first all-sky observations of 'polarised' light emitted by interstellar dust in the Milky Way.
Light is a very familiar form of energy and yet some of its properties are all but hidden to everyday human experience. One of these – polarisation – carries a wealth of information about what happened along a light ray's path, and can be exploited by astronomers.
Usually, these fields can vibrate at all orientations. However, if they happen to vibrate preferentially in certain directions, we say the light is 'polarised'. This can happen, for example, when light bounces off a reflective surface like a mirror or the sea. Special filters can be used to absorb this polarised light, which is how polarised sunglasses eliminate glare.
In space, the light emitted by stars, gas and dust can also be polarised in various ways. By measuring the amount of polarisation in this light, astronomers can study the physical processes that caused the polarisation.
In particular, polarisation may reveal the existence and properties of magnetic fields in the medium light has travelled through.
The map presented here was obtained using detectors on Planck that acted as the astronomical equivalent of polarised sunglasses. Swirls, loops and arches in this new image trace the structure of the magnetic field in our home galaxy, the Milky Way.
In addition to its hundreds of billions of stars, our Galaxy is filled with a mixture of gas and dust, the raw material from which stars are born. Even though the tiny dust grains are very cold, they do emit light but at very long wavelengths – from the infrared to the microwave domain. If the grains are not symmetrical, more of that light comes out vibrating parallel to the longest axis of the grain, making the light polarised.
If the orientations of a whole cloud of dust grains were random, no net polarisation would be seen. However, cosmic dust grains are almost always spinning rapidly, tens of millions of times per second, due to collisions with photons and rapidly moving atoms.
Then, because interstellar clouds in the Milky Way are threaded by magnetic fields, the spinning dust grains become aligned preferentially with their long axis perpendicular to the direction of the magnetic field. As a result, there is a net polarisation in the emitted light, which can then be measured.
In this way, astronomers can use polarised light from dust grains to study the structure of the Galactic magnetic field and, in particular, the orientation of the field lines projected on the plane of the sky.
In the new Planck image, darker regions correspond to stronger polarised emission, and the striations indicate the direction of the magnetic field projected on the plane of the sky. Since the magnetic field of the Milky Way has a 3D structure, the net orientation is difficult to interpret if the field lines are highly disorganised along the line of sight, like looking through a tangled ball of string and trying to perceive some net alignment.
However, the Planck image shows that there is large-scale organisation in some parts of the Galactic magnetic field.
The dark band running horizontally across the centre corresponds to the Galactic Plane. Here, the polarisation reveals a regular pattern on large angular scales, which is due to the magnetic field lines being predominantly parallel to the plane of the Milky Way.
The data also reveal variations of the polarisation direction within nearby clouds of gas and dust. This can be seen in the tangled features above and below the plane, where the local magnetic field is particularly disorganised.
Planck's Galactic polarisation data are analysed in a series of four papers just submitted to the journal Astronomy & Astrophysics, but studying the magnetic field of the Milky Way is not the only reason why Planck scientists are interested in these data. Hidden behind the foreground emission from our Galaxy is the primordial signal from the Cosmic Microwave Background (CMB), the most ancient light in the Universe.
generated in the Universe immediately after its birth.
See the full article, with "more information", here.


Prep Day: In a large resealable plastic bag, combine the onion powder, garlic powder, chipotle chile powder, salt, and brown sugar. Place tenderloins in bag and shake, coating meat evenly. Freeze after well coated.
Serve Day: Thaw. Preheat grill for medium-high heat. Lightly oil grill grate, and arrange meat on grate. Cook for 20 minutes, turning meat every 5 minutes. Remove from grill, let stand for 5 to 10 minutes before serving.
Prep Day: Mix marinade together in plastic bag. Add pork chops. Freeze.
Server Day: Thaw. Grill 10-12 minutes per side or until 145 degrees internal temp. Serve with mango salsa (you provide), if desired.
Prep Day: In a mini food processor, combine the garlic, oregano, paprika, chile powder, curry and salt and process until the garlic is chopped. Add the vinegar and olive oil and process to a paste. Rub the marinade onto the turkey cutlets, bag and freeze.
Serve Day: Thaw turkey in refrigerator for 24 hours. Light a grill. Scrape the marinade off of the turkey cutlets. Brush the cutlets with vegetable oil and grill over moderately high heat, turning once, until lightly charred and cooked through, about 5 minutes total. Prepare rice and black beans per package directions.
Prep Day: Brown sausage in a skillet; drain. In a bowl, combine sausage, cheese and tomatoes. Cook eggs in the skillet. Add eggs to sausage mixture and mix thoroughly. Divide mixture evenly among tortillas and roll tightly. Seal tortillas by cooking for one to 2 minutes on a hot griddle sprayed with non-stick vegetable spray.
Wrap the burrito in a piece of parchment, foil or plastic wrap using the same method that was used to roll up the tortilla. Secure with tape if desired and label the burrito with its contents. Place the wrapped burritos in a freezer bag.
Serve Day: Place the burrito on a plate (without wrapper) and microwave for one minute on high. Check to see if the burrito is heated through and microwave longer if needed.
Prep Day: Combine all marinade ingredients well. Coat chicken pieces in marinade paste. Marinate from 1 hour, or up to overnight in the refrigerator.
Serve Day: thaw. Grill over medium coals until browned, about 15 minutes each side.
Prep Day: In a small bowl, whisk together brown sugar, soy sauce, sesame oil, red pepper flakes and ginger. Place in a small freeze able container. Package up garlic, beef and onion individually.
Serve Day: Heat vegetable oil in a large skillet over medium high heat. Add garlic and cook, stirring constantly, until fragrant, about 1 minute. Add ground beef and cook until browned, about 3-5 minutes, making sure to crumble the beef as it cooks; drain excess fat. Stir in soy sauce mixture and green onions until well combined, allowing to simmer until heated through, about 2 minutes.
Prep Day Directions: Add crushed red pepper, salt, pepper and garlic. Sauté long enough for garlic to caramelize and red pepper to release its flavor into the oil.
Add sliced chicken and sauté briefly to coat in garlic and spices.
Add marinara first, and then alfredo sauce. Bring to a simmer. Cook until sauce thickens slightly and chicken is cooked to an internal temperature of 165˚. Remove from heat.
Add butter and peas into the sauce.
Cook pasta according to package directions. Toss in sauce. You may garnish with more crushed red pepper if you'd like.
Serve Day Directions: You can thaw the bag and heat it up on the stove top OR cook in crockpot on low for 6-8 hours. Cook pasta and mix with chicken and sauce. Enjoy.
Prep Day: Label your freezer bag. To your freezer bag, add all ingredients. Add chicken to the freezer bag last so it's the first ingredient poured into your crockpot. Remove as much air from the freezer bag as possible, seal, and lay flat in your freezer.
Serve Day: The night before cooking, move frozen bag to your refrigerator to thaw. The morning of cooking, pour contents of freezer bag into your crockpot. Cook on "low" setting for 4-6 hours, or until chicken is cooked through.
NOTE: Meal Swappers ONLY please vote on the July 2015 Menu!


No detection capability demonstrated for this procedure, though the Interactive Shell was used to analyze the PowerShell execution and WinEnum Available Shares was observed. Interactive Shell was not by itself considered telemetry, but the analyst can retrieve additional Windows Logs to enhance baseline Endgame functionality.
No detection capability demonstrated for this procedure, though the Interactive Shell was used to analyze the PowerShell execution and WinEnum Mapped Network Drives was observed. Interactive Shell was not by itself considered telemetry, but the analyst can retrieve additional Windows Logs to enhance baseline Endgame functionality.


Kelly Walsh, a 20-year human resource veteran, formed 1SmartLife, to offer convenient and affordable personal coaching to executives nationwide and once again joins Enterprise Radio. Kelly will share how to juggle personal relationships and professional ambitions and learn who can benefit from life coaching.
Kelly Walsh, a 20-year human resource veteran, formed 1SmartLife, to offer convenient and affordable personal coaching to executives nationwide and joins Enterprise Radio.


DEAR DR. ROACH: I love fish and chips. I eat them once a month. I have tuna and other fish throughout the month as well. Quite often, the fishy odors linger for days until all remnants have left my body. Is there anything I can do to counteract the smell? I feel that others can tell when I have eaten fish. The odor comes from my mouth, my urine and my feces. — J.C.A.
ANSWER: Fish, particularly deep-saltwater fish, contain a substance called trimethylamine oxide. After fish die, it is converted by bacteria and enzymes in the fish to trimethylamine, which is largely responsible for the "fishy" odor; it gets stronger over time. Trimethylamine in humans is excreted through sweat in addition to urine and feces. People have different amounts of the enzyme that breaks down TMA so there's a variance in the noticeable effect of fishy breath and sweat after consuming fish. A very few people lack the enzyme entirely.
TMA can be washed off of fish, and also can be broken down by acid, such as in lemons. Rinsing fish before cooking or using lemon during or after cooking will lessen the odor effect on you.
Other foods also may cause an evident odor in the sweat and urine. Cruciferous vegetables like broccoli and asparagus can change the odor of urine and sweat, as can garlic, onions and some spices. Alcohol, especially in excess, can be picked up by people with sharp noses. Men who ate no meat for two weeks were found to have a "more pleasant" body odor than those who did.
DEAR DR. ROACH: A friend told me she was given a bowel regimen for a minimally invasive procedure. She said that she didn't have to drink any solution the night before, and her doctor and nurse practitioner never discussed the issue. Can you tell us what a "bowel regimen" is? — K.C.H.
ANSWER: A regimen (not "regime," that's a government; and not "regiment," that's an army unit) is simply a prescribed treatment. In the context of an upcoming procedure like a colonoscopy, a bowel regimen means using medication to evacuate the colon. The colon needs to be empty so the examiner can see the lining of the wall.
The most common bowel regimens are nonabsorbable large molecules in a solution that has a salt balance similar to that of the body. These pass through the colon fast enough to wash away all the contents of the colon, preferably without affecting the salt levels of the blood, which must be kept tightly regulated. These can be low volume (2 liters) or high volume (4 liters). They are effective, but don't taste particularly pleasant (drinking them cold or with flavoring agents can help). In practical terms, this means a fair amount of diarrhea.
If your friend didn't drink a solution, she probably had sodium phosphate tablets. These are not recommended for people over 65; those who have heart or kidney problems; or people who take diuretics, some heart medicines or anti-inflammatories. They also can damage the lining of the intestines. Given all of the concerns with this preparation, I seldom see it used.


 Join ARC's Greg Carroll and Mike Pagán as they celebrate Charlie Parker and their new label release in Kansas City at Westport Coffeehouse Theater  Available soon at all of the major retail stores.
368 songs, 41 hours 28 minutes LISTEN ON COMPUTERS  Listen to ARC Label music on Spotify! LISTEN ON MOBILE DEVICES  Listen to ARC Label music on Spotify!


This little trio of rustic wood signs started in January when I picked my One-Word for 2015…Love.
I used vintage silverware to spell LOVE and made a rustic pallet wood sign for the background. I didn't sand the pallet wood for that sign because I wanted to remember that love isn't always smooth. Often times, to love someone, means going through some rough spots.
My HOPE sign was a little different. I started by making the same pallet wood backdrop, but this time, instead of leaving the wood rough, I sanded all rough places and sharp edges and used a teal stain. Because to me, that's what hope does, soften up the sharp edges of life…also, if hope was a color, (I think) it would be teal…teal makes my heart sing.
My last sign of course, had to be FAITH.
To go along with the easy wood frame, my FAITH sign is made with rustic wood letters. I picked the wood letters on the wood frame because it was a sturdy and strong combination. And our faith, is the strength and foundation of our family.
It's super easy and like I said, if you learn to make one or two frames/signs, you'll be able to use them to do so many projects around the house!
Sand over all edges…I like my edges to be smooth and a little bit rounded—that makes the piece look more rustic, like the wood has been around a while.
Now- stain everything. I used Varthane Weathered Gray.
For more information on making this sign, go HERE.
I'm really happy with my Faith-Hope-Love signs in the breakfast room, each one different, like the words they represent, but each one works well with the other.
« From New to Vintage Crate Makeover!
I love your signs, and your significance of how/why each was made is such an example of how each word should be viewed. Thank you, with love!


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Premium Home Chevron icon It indicates an expandable section or menu, or sometimes previous / next navigation options. Strategy
A former barista reveals how she started a journal business on the side and scaled it to make $500,000 in sales this year
Phil Rosen
Taylor Ruotsala, founder of Never Stay Stagnant, with her journals. She's sold over 300 a month since December.
Taylor Ruotsala
Taylor Ruotsala, 28, founded self-help journal company Never Stay Stagnant in 2018.
She primarily uses Facebook ads and Instagram for marketing and scaling her business.
On track to clear $500,000 in sales for 2021, Ruotsala is aiming to make $1 million next year.
By the time she'd quit her full-time job at a coffee shop in January 2021, Taylor Ruotsala, 28, was already making nearly $9,000 per month from her self-help journal company, Never Stay Stagnant, that she started in 2018.
After multiple months of selling over 300 journals (to a 90% female demographic), she decided to fully invest her time and energy into her business.
Ruotsala told Insider she initially created the journals for herself because she couldn't find any on the market that included the specific things she wanted.
"I just wanted something that wasn't so repetitive, something that tracked my sleep, my water, my morning routine," Ruotsala said. "Something that could take me to the next level and push me, like my own personal mentor."
This year, she's on track to clear $500,000 in sales. Her company's Instagram page has over 6,000 followers.
Here's how she scaled her company.
Finding an audience through friends
Never Stay Stagnant journals.
Ruotsala first realized she had a potential business when several of her friends asked her to print them copies, too — so she built a website and refined her designs.
But nothing happened.
"I'd get one or two sales every now and then, but I wasn't doing anything" with the website, Ruotsala said. "I thought that's how businesses worked. You just built a site and people would come to you on their own."
"For women especially, a lot of us are held back from starting something because of a lack of confidence," Ruotsala added. "There's not as many women CEOs and leaders, so less women push themselves to that level."
Getting into social-media marketing
A post shared by Never Stay Stagnant (@neverstaystagnant)
In early 2020, Ruotsala began pushing to get her company off the ground. "I was working so hard in my job, making other people money, that I realized I could work this hard for my own business instead and see what happens," Ruotsala said.
She started posting regularly on her company's social-media accounts and began researching how to leverage social-media advertising.
"I literally Googled my way into learning about Facebook ads," Ruotsala said. "I started with a budget of a few dollars a day on Facebook, and by April [2020] I was selling about a journal every other day or so."
As she began selling more journals, Ruotsala increased her daily budget on Facebook ads. In May 2020, she spent about $12 per day on ads and sold 36 journals. By July, she'd increased her spending to about $18 per day — she sold 108 journals that month.
When she increased to $115 per day by December, she'd strung together multiple months of 300 journals sold.
"So in December [2020], I was still working in my full-time job and doing my business on the side, but I was making way more working less than 10 hours a week on the journals than I was doing 40 hours at my job," Ruotsala said.
Keeping up with demand
As Never Stay Stagnant gained more followers, the website garnered more traffic, and she had to print more journals to keep in stock. Ruotsala uses Amazon publishing services for orders she receives on Amazon and a local printing company in Thousand Oaks, California, for orders made through the company website.
Fully stocked, she keeps 1,600 journals in a storage unit near her house that she packages and ships out herself, sometimes with help from friends and family.
She bumped up her ad spending to $120 in January 2021 and then $200 in February, which brought in about $17,000 each month. She was scaling up her ad spending every five days, and by April 2020, she was spending about $500 per day on Facebook ads.
She made over $50,000 that month, selling over 40 journals per day.
While the product itself has proven popular, Ruotsala believes the positive message her company conveys is just as critical.
"You can't think of it as selling a product because really you should be selling a story," Ruotsala said. "People want to support people, not a product. So when you match your story to your product, customers can really get behind that. It's the story behind something that makes it so impactful."
Striving for seven figures
Ruotsala said she's aiming to hit $1 million in sales in 2022. And she wants her journal to help other women achieve their ambitions, too.
"Whatever it is, just start," Ruotsala said. "Build a website. Invest in yourself and your brand. Write things down and share your story with people."
Now, Ruotsala is working on a children's journal to help younger audiences develop goals and gain confidence in school. This will be her third journal on her website.
"I think my journals help women become happy with themselves and make them proud of the life they live," Ruotsala said. "I hope my journals point out the amazing things that people do each day even if it isn't building a huge business or being famous."
NOW WATCH: How Toms went from a $625 million company to being taken over by its creditors
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Contributor 2021
Lauryn Haas
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redpajama_set_name: RedPajamaCommonCrawl


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South Africa under the pump in ODI series
South Africa go into a three-match ODI series against England this week in a precarious position, needing to secure a whitewash if they are to make sure of automatic qualification for this year's World Cup.
South Africa are languishing in the World Cup Super League standings and are chasing the last available automatic qualifying berth for the tournament in India later this year - along with Ireland, Sri Lanka and the West Indies.
They sit in 11th place in the standings, having forfeited three ODIs against Australia this month in order to make room on the calendar for Cricket South Africa's new Twenty20 league, but can make 100 per cent sure of qualification if they beat England 3-0 and then win their last two qualifying ODIs in March and April at home to the Netherlands, who are bottom of the 13-team table.
Any slip up opens the door for one of the other chasing teams to qualify and could force South Africa, who have been to four semi-finals in eight World Cup appearances, into the ignominy of a having to play in a pre-qualifying tournament in mid-year.
The West Indies are eighth in the standings but have completed their Super League program. Sri Lanka must win two of three ODIs in New Zealand in March to overtake them while Ireland must win all three of their May series against already-qualified Bangladesh if they are to stand any chance of a top-eight finish.
If both Ireland and Sri Lanka do not win all their remaining three games, then South Africa's task is made easier but they still need to win a minimum of three victories to ensure automatic qualification to the World Cup, which will be held in October and November and comprises of 10 teams.
The Super League is the main qualification pathway for the tournament with the top seven sides, along with hosts India, gaining direct entry into the tournament. The other two are decided from the play-off tournament in Zimbabwe in mid-year.
South Africa go into the series against England with a new coaching line-up after Mark Boucher quit following November's T20 World Cup.
Shukri Conrad, who was named as South Africa's Test coach earlier this month, will take charge of the ODI squad against England while new white-ball coach, Rob Walter, finishes his commitments with the Central Stags in New Zealand.
Perth rescue ALM draw from 10-man Phoenix


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Mystery of Jupiter's powerful X-ray auroras finally solved
By Charles Q. Choi
The giant planet's auroras aren't so different than those on Earth
Overlaid images of Jupiter's pole from NASA's satellite Juno and NASA's Chandra X-ray telescope. Left shows a projection of Jupiter's Northern X-ray aurora (purple) overlaid on a visible Junocam image of the North Pole. Right shows the Southern counterpart. (Image credit: NASA Chandra/Juno Wolk/Dunn)
Mysterious flares of X-rays from Jupiter's auroras suggest that the giant planet's "northern lights" may possess unexpected similarities with those of Earth, a new study finds.
Auroras, the shimmering displays of radiance known as the northern or southern lights on Earth, are seen above the poles of a number of planets across the solar system. These dancing lights are produced when energetic particles from the sun or other celestial bodies slam into a planet's magnetosphere — the area controlled by a world's magnetic field — and flow down its magnetic field lines to collide with molecules in its atmosphere.
Jupiter's magnetic field is extremely strong — about 20,000 times more powerful than Earth's — and therefore its magnetosphere is extremely large. If that alien magnetosphere were visible in the night sky, it would cover a region several times the size of our moon. As such, Jupiter's auroras are much more powerful than Earth's, releasing hundreds of gigawatts — enough to briefly power all of human civilization.
In photos: Juno's amazing views of Jupiter
Jupiter's mysterious X-ray auroras have been explained, ending a 40-year quest for an answer. For the first time, astronomers have seen the way Jupiter's magnetic field is compressed, which heats the particles and directs them along the magnetic field lines down into the atmosphere of Jupiter, sparking the X-ray aurora. The connection was made by combining in-situ data from NASA's Juno mission with X-ray observations from ESA's XMM-Newton. (Image credit: ESA/NASA/Yao/Dunn)
Jupiter's auroras also emit unusual X-ray flares, ones that originate from electrically charged sulfur and oxygen ions spewed out by Jupiter's volcanic moon Io. Jupiter's X-ray auroras alone each release about a gigawatt, about what one power station on Earth might produce over several days. These X-ray auroras often pulse like clockwork, in regular beats a few dozen minutes long for dozens of hours.
The specific mechanisms driving these flares has long been a mystery. "For more than 40 years, we have been puzzling over what may cause Jupiter's spectacular X-ray aurora," study co-lead author Zhonghua Yao, a planetary scientist at the Key Laboratory of Earth and Planetary Physics in Beijing, told Space.com.
To uncover the sources of these flares, researchers used NASA's Juno probe, which orbits Jupiter, to inspect the giant planet's magnetosphere close up on July 16 and July 17, 2017. At the same time, they had the European Space Agency's XMM-Newton telescope, which orbits Earth, remotely analyze X-rays from Jupiter.
The scientists discovered that the X-ray flares are apparently triggered by regular vibrations of Jupiter's magnetic field lines. These vibrations generate planetary-scale waves of plasma — clouds of electrically charged particles — that send heavy ions "surfing" along the magnetic field lines until they smash into the planet's atmosphere, releasing energy in the form of X-rays.
Similar plasma waves help generate auroras on Earth. As such, despite Jupiter being so much bigger than Earth in every way — such as greater mass and diameter, more energy, stronger magnetic fields and faster rotation — "it seems like the processes responsible for Jupiter's ion aurora and Earth's ion aurora are the same," study co-lead author William Dunn, an astrophysicist at University College London, told Space.com. "This hints at a potential universal process for space environments."
It remains unclear why Jupiter's magnetic field lines vibrate regularly. Possibilities include interactions with the solar wind, or with high-speed plasma flows within Jupiter's magnetosphere, the researchers said.
The electrically charged particles the researchers spotted hurtling toward Jupiter's poles may not appear to have enough energy to generate X-ray aurora, "so they need to undergo some extra acceleration on the way," Yao said. "What are those extra acceleration processes?"
The scientists suggested that huge voltages that may exist above Jupiter's atmosphere may accelerate these electrically charged particles "towards the atmosphere with colossal energies," Dunn said. "These probably play a key role."
In the future, Yao suggested investigating other worlds to see if plasma waves might help drive auroras there as well. Similar activity may occur around Saturn, Uranus, Neptune and likely exoplanets as well, with different kinds of charged particles "surfing" the waves, he said.
The scientists detailed their findings online today (July 9) in the journal Science Advances.
Follow us on Twitter @Spacedotcom or Facebook.
Charles Q. Choi is a contributing writer for Space.com and Live Science. He covers all things human origins and astronomy as well as physics, animals and general science topics. Charles has a Master of Arts degree from the University of Missouri-Columbia, School of Journalism and a Bachelor of Arts degree from the University of South Florida. Charles has visited every continent on Earth, drinking rancid yak butter tea in Lhasa, snorkeling with sea lions in the Galapagos and even climbing an iceberg in Antarctica. Visit him at http://www.sciwriter.us


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Björn E. Engquist (né le  à Stockholm) est un mathématicien suédois. Il travaille actuellement à l'université du Texas à Austin.

Carrière
Il obtient son doctorat en analyse numérique de l'université d'Uppsala en 1975, où il enseigne les années suivantes en même temps qu'il occupe un poste de professeur à l'université de Californie à Los Angeles. En 2001, il part à l'université de Princeton où il occupe la chaire Michael Henry Stater de mathématiques et dirige le Program in Applied and Computational Mathematics. Il a également été professeur à l'Institut royal de technologie de Stockholm depuis 1993, et directeur du . Engquist occupe actuellement la chaire de Computational and Applied Mathematics à l' à l'université du Texas à Austin, après avoir quitté Princeton en 2005.

Publications

 avec Per Lötstedt, Olof Runborg : Multiscale Methods in Science and Engineering, Springer 2005
 avec Lötstedt, Runborg : Multiscale Modeling and Simulation in Science, Springer 2009
 Highly oscillatory problems, Cambridge University Press 2009
 avec Gregory Kriegsmann : Computational Wave Propagation, Springer 1997
 avec Stanley Osher, Richard Somerville : Large Scale computations in fluid mechanics, American Mathematical Society 1985
 avec  : Large Scale Scientific Computing, Birkhäuser 1987

Prix et distinctions
Il est conférencier invité au congrès international des mathématiciens en 1998 à Berlin avec une conférence intitulée Wavelet based numerical homogenization, après avoir déjà été invité en 1983 à Varsovie. En 1992 il donne une conférence plénière lors du Congrès européen de mathématiques intitulée Numerical approximation of hyperbolic conservation laws.

En 2016, il est lauréat du prix Chern. En 1982 il est le premier lauréat du prix James-Wilkinson, en 2012 il a reçu le prix George David Birkhoff et en 2011 le prix Peter-Henrici.

Il est membre de plusieurs sociétés savantes : l'Académie royale des sciences de Suède (1996), l'Académie royale des sciences de l'ingénieur de Suède (1997), l'Académie norvégienne des sciences et des lettres (2011) et l'Académie américaine des arts et des sciences (2015).

Références

Liens externes

Mathématicien suédois du XXe siècle
Mathématicien suédois du XXIe siècle
Naissance en juin 1945
Professeur à l'Institut royal de technologie
Professeur à l'université de Princeton
Professeur à l'université de Californie à Los Angeles
Professeur à l'université du Texas à Austin
Membre de l'Académie américaine des arts et des sciences
Membre de l'Académie royale des sciences de Suède
Membre de l'Académie norvégienne des sciences et des lettres
Lauréat du prix Birkhoff
Lauréat du prix Wilkinson
Lauréat du prix Peter-Henrici

redpajama_set_name: RedPajamaWikipedia


Our client has a fantastic opportunity for a Geotechnical Engineer to join their successful team based in Oldham.
* Write Phase 1, desk study reports including factual aspects, advising on geotechnical constraints, potential risk from contamination due to previous or adjoining land use and recommending the invasive investigation work phase.
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AOPEN Releases OpenSign Interactive In-Store Promoter
By AVNetwork Staff (Digital Signage Magazine, Systems Contractor News) 04 March 2013
AOPEN has just released OpenSign, a web based interactive digital marketing and signage platform for Android devices that allows retailers to easily install and manage a digital signage network.
OpenSign is purpose-built for different screen sizes, such as retail shelf displays and large promotional displays. It lets store owners actively manage digital content, without design experience, from any PC connected to the web. It also eliminates costly printing and the logistics of placing prints in the store, as well as enabling real-time offers and promotions to be run. Being cloud based, OpenSign can be easily integrated across multiple devices and platforms, including mobile devices. It also features local redundancy, meaning that content can still be displayed even if internet connection is lost.
Stephen Borg, director, global strategy and market development, AOPEN, says that OpenSign tackles the frustrations and costs of operating that retailers and store owners face when maintaining a digital signage network.
"As well as helping customers make a purchase decision, OpenSign captures customer data and retail patterns, which helps retailers understand what customers are looking for. This allows them to better promote products and services, creating new, highly targeted shopping experiences, in a cost-effective way," said Borg.
"OpenSign is a truly easy-to-manage, solution on a cost effective OS with competitive commercial grade hardware. It's a perfect product, designed and built for retailers. It also captures data and tracks results accurately."
OpenSign is Android-based, built using the same web application framework that powers websites such as Twitter and yellowpages.com. It's delivered globally with Rackspace, who are a premium provider of global data centers.
OpenSign represents a full digital signage ecosystem including: the OpenSign platform, dedicated devices and expert service. It can be used stand-alone or to complement existing signage networks. Its plug-in based API architecture allows integration with third party devices and applications, including existing CMS and e-commerce systems.
Being web-based, the signage can leverage any live feed you can get, such as: stock feeds, weather forecasts, POS data, social media feeds, loyalty programs and more. Designed with marketers in mind, OpenSign is also SEO friendly, allowing for social media integration and local area marketing via its easy to use content management system (CMS).
Growth in the worldwide digital signage market is forecast to exceed 40 percent in 2013, growing to U.S. $7 billion, according to IMS Research. Retail is the largest vertical, accounting for 25 percent of equipment and software sales. IMS predicts that retail will maintain its dominance, reaching nearly $2 billion USD in infrastructure sales by the end of 2015.
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Auditory evoked brainstem responses in patients with cronic hypozincemia: a clinical study.
Dr. med. Maria Cristina Lancia Cury Féres (São Paulo, Brazil)
Dr. med. Hélio Vanuchi (São Paulo, Brazil)
Some authors have postulate that sistemic zinc can be employed in the threatment of tinnitus, because a sub-clinical hypozincemia is suposed to promote this auditory disturbance. However, in the majority of the cases of tinnitus, this hypozincemia was not confirmed. There is not enough randomized studies that could show the relationship between zinc and tinnitus.
The main goals of this study were to evaluate a group of patients who have cronic hypozincemia, due to an extensive ressection of the small bowel, by means of the Auditory Evoked Responses, and to compare them with a control group, without auditory disorders, and with a group of patients who have tinnitus, without vertigo or hearing loss, in order to evaluate the functional features of the auditory pathways.
The patients were submitted to a detailled clinical observation, seric examination for zinc, magnesium, glucosis and tireoidean hormonies, audiometry, imitanciometry, speech discrimination tests and brainstem auditory evoked responses. The results of the three groups were statistically compared.
There were significative differences between the group with hypozincemia and the control group, concerning with the accoustic reflex for 1000 and 2000 Hz, and for the intervals III-V and I-V and for the amplitude of wave V, in the auditory evoked responses. There were no statistically significative differences between the groups with hypozincemia and with tinnitus, concerning with the auditory function.
We concluded that the nutritional disturbance of the patients with short small bowel, which includes hypozincemia, colaborates for the presence of a functional alteration in the central auditory system, and that this alteration makes this group of patients eletrophysiologically similar with those who have cronic tinnitus.


text:
Sunday Igboho: Let…
Sunday Igboho: Let justice prevail — Yoruba Council of Elders
Sunday Adeyemo aka Sunday Igboho
The Yoruba Council of Elders, YCE, has stated that if Sunday Adeyemo, also known as Sunday Igboho, has been detained, he should be given the right to defend himself.
The outburst followed reports that the popular Yoruba freedom warrior had been apprehended by security forces in Cotonou, West Africa.
Igboho was reportedly apprehended Monday night after fleeing Nigeria to avoid being apprehended by the country's secret police.
While speaking with the media about Igboho's alleged arrest, YCE Secretary-General Dr Kunle Olajide said: "For me, it has not been confirmed officially, and I am sure that the Department of State Security, DSS, would eventually confirm if it's genuine." And if that's the case, they'll have to follow the law to do an investigation."
"He should be charged in a court of law and be given the opportunity to defend himself. There should be no cause for concern until we receive formal confirmation that he has been arrested."
"However, I want to assure you that his detention will have no bearing on the Yoruba nation's movement. If the protesters are sincere in their beliefs, it should not prevent them from attaining their goals, according to Olajide.


Anastasia loves lists and she's creating a list of things she loves and things she hates. There are lots of things to classify: her soon-to-be-born baby brother, her ailing gradmother, the nutty and seductive Washburn Cummings, and her parents. For a fourth-grader, there's a lot to say.
A little odd to go back to middle reader material again, when I've been doing so much teen reading lately. Weirder to read a book that is actually contemporary with my childhood. The book dates itself in numerous places (teachers and students smoke in Anastasia's father's college classroom), but it has tremendous heart. A contemporary equivalent would be the Judy Moody series and that probably accounts for some of the enduring popularly of Lowry's writing. A nice diversion.


If anyone would like to discuss this, please feel free to reply.
Thanks a lot for the link. Hope to have u at SERES. cheers.
> a double-blind review process in place.
> workshop proceedings that are published online at CEUR-WS.
> Natasha Noy, Stanford University, USA.
> Li Ding, Rensselaer Polytechnic Institute, USA.
> John Bateman, Universität Bremen, Germany.
> Michael Kohlhase, Jacobs University, Germany.
> Raul Palma, Poznan University, Poland.
> Oscar Corcho, Universidad Politecnica de Madrid, Spain.
> Fabian Neuhaus, University of Maryland, USA.
> Christoph Lange, Jacobs University, Germany.
> Christopher Baker, University of New Brunswick, Canada.
> Nigam Shah, Stanford University, USA.
> Leyla Garcia, Bundeswehr University, Germany.


Does the name "Rob Joyce" ring a bell?
Chances are it does not, unless you work for his super-secretive team at the NSA — or heard him speak at January's Usenix Enigma security conference in San Francisco.
Joyce leads U.S. govenment's top hacking team, a division within the NSA known as Tailored Access Operations (TAO). The group is tasked with hacking the systems of foreign adversaries and allies alike.
With the NSA for more than 25 years, Joyce assumed the role of TAO leader shortly before Edward Snowden brought the agency's practices to the world's attention.
President Barack Obama wants computer science taught in all U.S. elementary, middle and high schools. And he wants upwards of $4 billion in spending to make it a reality.
In his weekly radio address, Obama said knowing how to use computers isn't enough. Knowing how to program them is critical.
"Today's auto mechanics aren't just sliding under cars to change the oil; they're working on machines that run on as many as 100 million lines of code. That's 100 times more than the Space Shuttle. Nurses are analyzing data and managing electronic health records. Machinists are writing computer programs," Obama said.
What spooks you more: Losing your online privacy or losing your chief source of income?
If your answer is the former, you're like 92% of respondents to a recent survey by the National Cybersecurity Alliance. In fact, data privacy topped the list of concerns. The "loss of personal income" ranked second (81 percent).
"Consumers are increasingly aware, interested and concerned about their privacy and they're acting on it," said Michael Kaiser, Executive Director National Cybersecurity Alliance. "However, if Internet users knew more, they would do more. The research points to an awareness-action shortfall that belies a growing confidence in Americans' personal ability to protect their online data.
For quick consumption of the findings, read this infographic from the TRUSTe/NCSA Consumer Privacy Index.
Distributed Denial of Service (DDoS) attacks are growing bigger, more frequent and more widespread, according to an annual security report by Arbor Networks.
According to SCMagazine.com, the Worldwide Infrastructure Security Report says the largest DDoS attack it recorded last year was 500 Gbps. In 2014, the largest recorded attack was 400 Gbps.
Private gun sales on Facebook, as well as Facebook-owned Instagram, are officially prohibited.
The Los Angeles Times reported that the ban strictly applies to "private transactions." Licensed gun sellers will not be affected.
Facebook has 1.59 billion monthly active users. Marijuana, pharmaceutical and illegal drug sales are already banned.
Gun control advocates celebrated their win, Reuters reported.


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Hamilton employer shifting to 4-day workweek as businesses rethink tradition
Hamilton | Ontario | Business | Latest News |
Published January 20, 2022 at 1:12 pm
DPAI Architecture Inc., which has an office in downtown Hamilton, is moving to a four-day workweek as businesses pivot from tradition. (DPAI Architecture Inc. photo)
With the COVID-19 pandemic forcing businesses to pivot from their normal work structures, many employers have been rethinking the traditional Monday to Friday, nine to five model altogether.
DPAI Architecture Inc., which has an office in downtown Hamilton, is ditching tradition entirely.
Founder and CEO David Premi announced that the company is trying out a four-day workweek.
"It comes as no surprise to anyone living on this planet that much has changed over the past two years," he wrote in a LinkedIn post. "We're collaborating differently now, and during the pandemic, we've reflected on how to make our work lives more meaningful and better integrated with our personal lives."
"In response to the changing workplace, we embark on a four-day workweek. This is an exciting endeavour for us and we believe that it will enhance the quality of service that we are able to provide to our clients," wrote Premi.
For four years researchers tracked 2,500 workers in Iceland who had their schedules reduced to four days a week. Their weekly hours were also reduced from 40 to 35 hours while their pay remained the same.
Bank of Canada raises key interest rate to the highest it has been since 2007
What another Bank of Canada rate hike could mean
Fiscal room tightening as economy teeters, associate finance minister says during Hamilton retreat
Researchers concluded that the changes improved the workers' well-being and productivity.
"Worker wellbeing dramatically increased across a range of indicators, from perceived stress and burnout to health and work-life balance," the report stated. Additionally, "productivity and service provision remained the same or improved across the majority of trial workplaces."
DPAI Architecture Inc. is behind the Gore Park project and has been a big player in the Hamilton area. Premi's team will also lead the renovations of the city's entertainment precinct.
DPAI says its business hours will still be Monday to Friday, from 8:30 a.m. to 5 p.m. Its employees will work a 36-hour week with a two-shift rotation; half of the team will be off on Mondays and the other half will get Fridays off.
"We understand that everyone has unique circumstances, so continuously provide accommodations that allow our team to thrive personally and professionally," wrote DPAI. "Giving our team more time to recharge will result in happier, healthier people and ultimately translate to the best solutions and service for our clients."
Employees will also have the ability to flex their time and work both from home and in the office, depending on individual needs.


Area/Size : 1435 Sq.ft To 3050 Sq.ft.
Area : 2200 Sq.ft and 3050 Sq.ft.
173 Villas / 13 Acres.
Royal Sunnyvale an establishment by M S Shelters which made it grounds in the year 2007. M S Shelters has rapidly and innovatively created a new position in construction and developments business. Till now the group has completed three projects with one 0n-going project with two coming project.
Royal Sunnyvale has a well settled neighbourhood like Sri Shabari Juice and Candments, Expat Vida-Bangalore, Alliance University, Alliance School of Law and Settahali Lake. It has well road connectivity too like Chandapura Anekal Road, Thattanhalli Main Road, Anekal Railway and Attibele-Anekal Road.
Royal Sunnyvale offers you 3 BHK & 4 BHK Villas and the building offers 173 Villas within 13 Acres of land. Royal Sunny Vale offers you an area of 1435 Sq.ft to 3050 Sq.ft.
Royal Sunnyvale offers you and garden with an entrance lobby with a living area and dining area with a sit out in the garden area. The 3 BHK Villas offers you three master bedrooms with wit utility space dressing space and balcony sit-out. A separate utility room too with a puja room. The kitchen offers you a utility space with storage area and servant rooms.
The 4 BHK Villa offers you a living area with and separate dining with a wit and balcony sit-out and with a garden sit-out too. It offers you 4 BHK with three master bedrooms with dressing space, powder room with balconies. A single bedroom with dressing space. A spacious lobby with utility area, puja room, and servant room. The kitchen offers you a separate utility area.
It offers you all the basic amenities like Entry Lounge, Coffee Bar, Health Club, Swimming Pool, Indoor Games, Snooker, Table Tennis, and Squash Court. It offers you 24/7 Water Supply, 24/7 Power Backup Facility with Video Door Phone Facility.
The exteriors as well as interiors are well designed the flooring is made up of vitrified tiles with ceramic tiles in balcony, garden, powder room and in lobby area. The doors are made up of teak wood with teak wood frame. The toiletry fittings are made up by jacquar and the electrical fittings are done with copper wiring with all the safeguard system.
* Polished teakwood main door frame with modular teakwood shutter.
* Internal doors with hardwood frame and modular shutters.
* Windows with 3/2 track aluminium frame and glass shutters with MS safety grill.
* MS railings for staircase & balcony.
* Vitrified tiles flooring for living, dining and kitchen.
* Ceramic tiles above the granite platform up to 2 ft. height.
* Good quality anti skid tiles for the toilet flooring.
* Sadarhalli granite for staircase.
* Acrylic emulsion paint for internal walls and the ceiling.
* Acrylic weather proof emulsion paint for the external walls.
* Good quality glazed tiles dadoing till 7 ft height.
* Standard quality sanitary & wash basin.
* Jaguar / equivalent plumbing fixtures.
* 3 Kw / 5 Kw power.
* Computer, internet, TV and telephone points.
* Provision for solar water heater.
* 1000 KVA DG backup.
* Hydropneumatic water supply system with basic water treatment plant.
* ISI make concealed pipes.
* ISI make PVC pipes.


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Home > Legislation > 111th Congress > H.R.4746
H.R.4746 - To amend the Internal Revenue Code of 1986 to prevent pending tax increases, and for other purposes.111th Congress (2009-2010)
Rep. Neugebauer, Randy [R-TX-19] (Introduced 03/03/2010)
House - Ways and Means
House - 03/03/2010 Referred to the House Committee on Ways and Means. (All Actions)
Cosponsors: H.R.4746 — 111th Congress (2009-2010)All Information (Except Text)
Sponsor: Rep. Neugebauer, Randy [R-TX-19] | Cosponsor statistics: 76 current - includes 0 original
Rep. Jenkins, Lynn [R-KS-2] 03/19/2010
Rep. Barton, Joe [R-TX-6] 03/19/2010
Rep. Manzullo, Donald A. [R-IL-16] 03/19/2010
Rep. Olson, Pete [R-TX-22] 03/19/2010
Rep. Chaffetz, Jason [R-UT-3] 03/19/2010
Rep. Campbell, John [R-CA-48] 03/19/2010
Rep. Bartlett, Roscoe G. [R-MD-6] 03/19/2010
Rep. Akin, W. Todd [R-MO-2] 03/19/2010
Rep. Pitts, Joseph R. [R-PA-16] 03/19/2010
Rep. Griffith, Parker [R-AL-5] 03/19/2010
Rep. Gohmert, Louie [R-TX-1] 03/19/2010
Rep. Conaway, K. Michael [R-TX-11] 03/19/2010
Rep. Bishop, Rob [R-UT-1] 03/19/2010
Rep. King, Steve [R-IA-5] 03/19/2010
Rep. Hensarling, Jeb [R-TX-5] 03/19/2010
Rep. Pence, Mike [R-IN-6] 03/19/2010
Rep. Issa, Darrell E. [R-CA-49] 03/19/2010
Rep. Jordan, Jim [R-OH-4] 03/19/2010
Rep. Price, Tom [R-GA-6] 03/19/2010
Rep. Marchant, Kenny [R-TX-24] 03/19/2010
Rep. Posey, Bill [R-FL-15] 03/19/2010
Rep. McClintock, Tom [R-CA-4] 03/19/2010
Rep. Fallin, Mary [R-OK-5] 03/25/2010
Rep. Gerlach, Jim [R-PA-6] 03/25/2010
Rep. Souder, Mark E. [R-IN-3] 03/25/2010
Rep. Burton, Dan [R-IN-5] 03/25/2010
Rep. Duncan, John J., Jr. [R-TN-2] 03/25/2010
Rep. Schock, Aaron [R-IL-18] 03/25/2010
Rep. Blackburn, Marsha [R-TN-7] 03/25/2010
Rep. Lamborn, Doug [R-CO-5] 03/25/2010
Rep. Hall, Ralph M. [R-TX-4] 04/14/2010
Rep. McCaul, Michael T. [R-TX-10] 04/14/2010
Rep. Simpson, Michael K. [R-ID-2] 04/14/2010
Rep. Alexander, Rodney [R-LA-5] 04/14/2010
Rep. Latta, Robert E. [R-OH-5] 04/14/2010
Rep. Wilson, Joe [R-SC-2] 04/14/2010
Rep. Paul, Ron [R-TX-14] 04/14/2010
Rep. Poe, Ted [R-TX-2] 04/14/2010
Rep. Franks, Trent [R-AZ-2] 04/14/2010
Rep. Lee, Christopher J. [R-NY-26] 04/15/2010
Rep. Rehberg, Denny [R-MT-At Large] 04/15/2010
Rep. Moran, Jerry [R-KS-1] 04/15/2010
Rep. Bachmann, Michele [R-MN-6] 04/15/2010
Rep. Miller, Gary G. [R-CA-42] 04/29/2010
Rep. Shimkus, John [R-IL-19] 04/29/2010
Rep. Tiahrt, Todd [R-KS-4] 04/29/2010
Rep. Calvert, Ken [R-CA-44] 04/29/2010
Rep. Garrett, Scott [R-NJ-5] 05/20/2010
Rep. Barrett, J. Gresham [R-SC-3] 07/14/2010
Rep. Heller, Dean [R-NV-2] 07/14/2010
Rep. Buchanan, Vern [R-FL-13] 07/22/2010
Rep. Rogers, Harold [R-KY-5] 07/22/2010
Rep. Myrick, Sue Wilkins [R-NC-9] 07/29/2010
Rep. Stearns, Cliff [R-FL-6] 07/29/2010
Rep. Lance, Leonard [R-NJ-7] 07/30/2010
Rep. Broun, Paul C. [R-GA-10] 07/30/2010
Rep. Roe, David P. [R-TN-1] 07/30/2010
Rep. Sullivan, John [R-OK-1] 07/30/2010
Rep. Bilbray, Brian P. [R-CA-50] 07/30/2010
Rep. Sensenbrenner, F. James, Jr. [R-WI-5] 07/30/2010
Rep. LoBiondo, Frank A. [R-NJ-2] 09/16/2010
Rep. Fleming, John [R-LA-4] 09/16/2010
Rep. Gingrey, Phil [R-GA-11] 09/16/2010
Rep. Rooney, Thomas J. [R-FL-16] 09/16/2010
Rep. Kline, John [R-MN-2] 09/16/2010
Rep. Shadegg, John B. [R-AZ-3] 09/16/2010
Rep. Schmidt, Jean [R-OH-2] 09/16/2010
Rep. Carter, John R. [R-TX-31] 09/16/2010
Rep. Capito, Shelley Moore [R-WV-2] 09/29/2010
Rep. Wittman, Robert J. [R-VA-1] 09/29/2010
Rep. Coffman, Mike [R-CO-6] 11/15/2010
Rep. Foxx, Virginia [R-NC-5] 12/02/2010
Rep. McKeon, Howard P. "Buck" [R-CA-25] 12/02/2010
Rep. Biggert, Judy [R-IL-13] 12/02/2010
Rep. Luetkemeyer, Blaine [R-MO-9] 12/02/2010
Rep. McMorris Rodgers, Cathy [R-WA-5] 12/07/2010
03/19/2010 - Rep. Jenkins, Lynn [R-KS-2]
03/19/2010 - Rep. Barton, Joe [R-TX-6]
03/19/2010 - Rep. Manzullo, Donald A. [R-IL-16]
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03/19/2010 - Rep. Bartlett, Roscoe G. [R-MD-6]
03/19/2010 - Rep. Akin, W. Todd [R-MO-2]
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03/19/2010 - Rep. Gohmert, Louie [R-TX-1]
03/19/2010 - Rep. Conaway, K. Michael [R-TX-11]
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03/19/2010 - Rep. King, Steve [R-IA-5]
03/19/2010 - Rep. Hensarling, Jeb [R-TX-5]
03/19/2010 - Rep. Pence, Mike [R-IN-6]
03/19/2010 - Rep. Issa, Darrell E. [R-CA-49]
03/19/2010 - Rep. Jordan, Jim [R-OH-4]
03/19/2010 - Rep. Price, Tom [R-GA-6]
03/19/2010 - Rep. Marchant, Kenny [R-TX-24]
03/19/2010 - Rep. Posey, Bill [R-FL-15]
03/19/2010 - Rep. McClintock, Tom [R-CA-4]
03/25/2010 - Rep. Fallin, Mary [R-OK-5]
03/25/2010 - Rep. Gerlach, Jim [R-PA-6]
03/25/2010 - Rep. Souder, Mark E. [R-IN-3]
03/25/2010 - Rep. Burton, Dan [R-IN-5]
03/25/2010 - Rep. Duncan, John J., Jr. [R-TN-2]
03/25/2010 - Rep. Schock, Aaron [R-IL-18]
03/25/2010 - Rep. Blackburn, Marsha [R-TN-7]
03/25/2010 - Rep. Lamborn, Doug [R-CO-5]
04/14/2010 - Rep. Hall, Ralph M. [R-TX-4]
04/14/2010 - Rep. McCaul, Michael T. [R-TX-10]
04/14/2010 - Rep. Simpson, Michael K. [R-ID-2]
04/14/2010 - Rep. Alexander, Rodney [R-LA-5]
04/14/2010 - Rep. Latta, Robert E. [R-OH-5]
04/14/2010 - Rep. Wilson, Joe [R-SC-2]
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04/14/2010 - Rep. Poe, Ted [R-TX-2]
04/14/2010 - Rep. Franks, Trent [R-AZ-2]
04/15/2010 - Rep. Lee, Christopher J. [R-NY-26]
04/15/2010 - Rep. Rehberg, Denny [R-MT-At Large]
04/15/2010 - Rep. Moran, Jerry [R-KS-1]
04/15/2010 - Rep. Bachmann, Michele [R-MN-6]
04/29/2010 - Rep. Miller, Gary G. [R-CA-42]
04/29/2010 - Rep. Shimkus, John [R-IL-19]
04/29/2010 - Rep. Tiahrt, Todd [R-KS-4]
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05/20/2010 - Rep. Garrett, Scott [R-NJ-5]
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07/30/2010 - Rep. Lance, Leonard [R-NJ-7]
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07/30/2010 - Rep. Roe, David P. [R-TN-1]
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07/30/2010 - Rep. Bilbray, Brian P. [R-CA-50]
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09/16/2010 - Rep. Carter, John R. [R-TX-31]
09/29/2010 - Rep. Capito, Shelley Moore [R-WV-2]
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11/15/2010 - Rep. Coffman, Mike [R-CO-6]
12/02/2010 - Rep. Foxx, Virginia [R-NC-5]
12/02/2010 - Rep. McKeon, Howard P. "Buck" [R-CA-25]
12/02/2010 - Rep. Biggert, Judy [R-IL-13]
12/02/2010 - Rep. Luetkemeyer, Blaine [R-MO-9]
12/07/2010 - Rep. McMorris Rodgers, Cathy [R-WA-5]
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This print of the original is a full colour lithoprint with raised U.V. detail. Each print is printed on 400gsm lumisilk paper and is signed and numbered by the artist. The artwork is an edition of 100 and measures 26 x 28½ inches.
Frame Details - Black Maple Shadow Frame with White Spacer and UV Plexi Glass.
Shipping and Handling is included. Please note that these limited edition prints can take up to 10 business days to ship.


text:
All news, UNITE - Latest
Liverpool airport's success crucial to region's economic welfare as thousands of aviation jobs hang by a thread
30 May 2020 Steve Leave a comment
New research, commissioned by Unite the union, has revealed that securing the future of Liverpool John Lennon airport is crucial to the wellbeing of the region's economy.
Liverpool airport generates around £410 million across the North West of England every year and provides direct and indirect employment for more than 10,000 people in the North West.
Unite is warning that without urgent action by central government to stabilise the aviation sector, jobs dependent on Liverpool airport, including crew, ground staff, engineers and associated retail, transport and other roles, will be swept away.
Unite has produced a blueprint of how the government should intervene across the entire aviation sector, including airlines and airports, to protect jobs and conditions of workers. Such loans would come with strict strings attached regarding executive pay, corporate governance and requiring strict environmental standards to be adopted to radically improve the industries carbon footprint.
The blueprint also recognises that in order to secure their future airports of the size of Liverpool may need a different ownership model in order to flourish, with public ownership or a public private partnership being an alternative.
Unite regional officer Mike Gaskell said: "Airports are hives of economic activity. Liverpool airport pumps £145 million into the city's economy and £410 million across North of England as a whole. The airport supports the jobs and livelihoods of scores of workers, from air crew to taxi drivers to shop staff.
"If these jobs go then a huge economic hole will open up in the Liverpool area and it could take decades to recover.
"Overnight, airports were effectively shut down by the government to protect the public's health, but we are now pleading with government to protect our area's long-term economic security.
"We are not asking for a giveaway, but for loans that will be repaid when the sector is back on its feet, and we have support for this from across the political spectrum.
"But the clock is ticking. It is more than two months since the chancellor promised that a support package would be forthcoming for aviation, however he has yet to deliver. The communities that rely on Liverpool airport for jobs and their prosperity cannot wait much longer."
Unite is calling on everyone whose work is connected to the airport or who is concerned about its future to email their MP and call for support for the airport and the UK's entire aviation sector.
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Apparently If You Tap These Spots 1x a Day For a Week THIS Is What Happens To Your Body!
Hey Dad, Are You Helping Your Child Have a Healthy Weight?
My name is Ray, and I'm obsessed with recovery. Maybe it's because I've seen how far the realm of recovery has come, or maybe it's because I myself have sustained a number of injuries. Regardless, I'm infatuated, and I spend most of my time looking for the best recovery tricks out there.
When you talk about vitamins and supplements, people often get the impression that it's all right to take as many as one wants. After all, they're supposedly good for the body, right?


Handheld Catering recently provided corporate catering in Menlo Park for the Precourt Institute for Energy at Stanford.
The Precourt Institute for Energy at Stanford (PIE) serves as the hub of a broad and deep network of experts from various scientific, technological, behavioral, and policy disciplines who are working independently and collaboratively to solve the world's most pressing energy problems.
Handheld has been honored to provide catering for PIE and SESI at their corporate events and for the most recent event we were presented with a unique and exciting event specific catering request, read about our unique dessert and the full event menu from our blog (click here to read more about our Chocoloate Mousse "Tank").
Handheld has an extensive selection of menu items to fit any palette and any unique dietary requirements. We would love to help you plan your Bay Area event catering. Consider allowing us to make your big night smoother, more relaxing, and delicious with our outstanding site-cooked foods. Call us at (408) 692-4782 or Contact Us Here.