logo
IIA researchers use commercial dish TV antennas to measure Sun's magnetic field

IIA researchers use commercial dish TV antennas to measure Sun's magnetic field

The Hindu5 hours ago

A team of scientists and engineers from the Indian Institute of Astrophysics (IIA) radio astronomy group has used a novel technique to measure the Sun's magnetic field using commercial dish TV antennas.
The technique involves measuring the magnetic field in the solar chromosphere, the region between the Sun's photosphere and corona, using the commercial dish TV antennas. The team demonstrated the technique recently.
According to the team, the antennas operate at a frequency of 11.2 GHz, which is in the radio astronomy band of the electromagnetic spectrum.
They said that this novel and unique effort has paved the way for regular measurement of the Sun's magnetic field from its surface to the outer layers of its atmosphere.
'Measurement of the magnetic field in the solar chromosphere is a key link to establish the connection between the Sun's surface and its corona from where the space weather disturbances originate. We are glad to have established a comparatively low-cost facility in the institute's Radio Astronomy Field Station in Gauribidanur for this purpose,' R. Ramesh, senior IIA professor and in charge of the Gauribidanur radio astronomy field station, told The Hindu.
Spurring other experiments
Prof. Ramesh said that the affordable set-up is expected to spur the educational institutions in the country to establish a similar facility on their campus, thereby paving the way for affordable astronomy that can provide valuable scientific quality data in addition to being a test bed to develop new technology within the country.
Students from BMS College of Engineering, Bengaluru, and Amrita Vishwa Vidyapeetam, Bengaluru Campus, were involved in the set-up in Gauribidanur as part of their academic project work.
He said the set-up will cost ₹20 lakh. 'This is a paltry sum compared to the budget required to establish a similar facility for measuring the Sun's magnetic field via conventional optical astronomy techniques, either from ground or space platforms,' he added.

Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

IIA researchers use commercial dish TV antennas to measure Sun's magnetic field
IIA researchers use commercial dish TV antennas to measure Sun's magnetic field

The Hindu

time5 hours ago

  • The Hindu

IIA researchers use commercial dish TV antennas to measure Sun's magnetic field

A team of scientists and engineers from the Indian Institute of Astrophysics (IIA) radio astronomy group has used a novel technique to measure the Sun's magnetic field using commercial dish TV antennas. The technique involves measuring the magnetic field in the solar chromosphere, the region between the Sun's photosphere and corona, using the commercial dish TV antennas. The team demonstrated the technique recently. According to the team, the antennas operate at a frequency of 11.2 GHz, which is in the radio astronomy band of the electromagnetic spectrum. They said that this novel and unique effort has paved the way for regular measurement of the Sun's magnetic field from its surface to the outer layers of its atmosphere. 'Measurement of the magnetic field in the solar chromosphere is a key link to establish the connection between the Sun's surface and its corona from where the space weather disturbances originate. We are glad to have established a comparatively low-cost facility in the institute's Radio Astronomy Field Station in Gauribidanur for this purpose,' R. Ramesh, senior IIA professor and in charge of the Gauribidanur radio astronomy field station, told The Hindu. Spurring other experiments Prof. Ramesh said that the affordable set-up is expected to spur the educational institutions in the country to establish a similar facility on their campus, thereby paving the way for affordable astronomy that can provide valuable scientific quality data in addition to being a test bed to develop new technology within the country. Students from BMS College of Engineering, Bengaluru, and Amrita Vishwa Vidyapeetam, Bengaluru Campus, were involved in the set-up in Gauribidanur as part of their academic project work. He said the set-up will cost ₹20 lakh. 'This is a paltry sum compared to the budget required to establish a similar facility for measuring the Sun's magnetic field via conventional optical astronomy techniques, either from ground or space platforms,' he added.

Earth Trapping More Heat Than Expected, Rate Doubled In 20 Years
Earth Trapping More Heat Than Expected, Rate Doubled In 20 Years

NDTV

time12 hours ago

  • NDTV

Earth Trapping More Heat Than Expected, Rate Doubled In 20 Years

Sydney: How do you measure climate change? One way is by recording temperatures in different places over a long period of time. While this works well, natural variation can make it harder to see longer-term trends. But another approach can give us a very clear sense of what's going on: track how much heat enters Earth's atmosphere and how much heat leaves. This is Earth's energy budget, and it's now well and truly out of balance. Our recent research found this imbalance has more than doubled over the last 20 years. Other researchers have come to the same conclusions. This imbalance is now substantially more than climate models have suggested. In the mid-2000s, the energy imbalance was about 0.6 watts per square metre (W/m2) on average. In recent years, the average was about 1.3 W/m2. This means the rate at which energy is accumulating near the planet's surface has doubled. These findings suggest climate change might well accelerate in the coming years. Worse still, this worrying imbalance is emerging even as funding uncertainty in the United States threatens our ability to track the flows of heat. Energy in, energy out Earth's energy budget functions a bit like your bank account, where money comes in and money goes out. If you reduce your spending, you'll build up cash in your account. Here, energy is the currency. Life on Earth depends on a balance between heat coming in from the Sun and heat leaving. This balance is tipping to one side. Solar energy hits Earth and warms it. The atmosphere's heat-trapping greenhouse gases keep some of this energy. But the burning of coal, oil and gas has now added more than two trillion tonnes of carbon dioxide and other greenhouse gases to the atmosphere. These trap more and more heat, preventing it from leaving. Some of this extra heat is warming the land or melting sea ice, glaciers and ice sheets. But this is a tiny fraction. Fully 90% has gone into the oceans due to their huge heat capacity. Earth naturally sheds heat in several ways. One way is by reflecting incoming heat off of clouds, snow and ice and back out to space. Infrared radiation is also emitted back to space. From the beginning of human civilisation up until just a century ago, the average surface temperature was about 14°C. The accumulating energy imbalance has now pushed average temperatures 1.3-1.5°C higher. Tracking faster than the models Scientists keep track of the energy budget in two ways. First, we can directly measure the heat coming from the Sun and going back out to space, using the sensitive radiometers on monitoring satellites. This dataset and its predecessors date back to the late 1980s. Second, we can accurately track the build-up of heat in the oceans and atmosphere by taking temperature readings. Thousands of robotic floats have monitored temperatures in the world's oceans since the 1990s. Both methods show the energy imbalance has grown rapidly. The doubling of the energy imbalance has come as a shock, because the sophisticated climate models we use largely didn't predict such a large and rapid change. Typically, the models forecast less than half of the change we're seeing in the real world. Why has it changed so fast? We don't yet have a full explanation. But new research suggests changes in clouds is a big factor. Clouds have a cooling effect overall. But the area covered by highly reflective white clouds has shrunk, while the area of jumbled, less reflective clouds has grown. It isn't clear why the clouds are changing. One possible factor could be the consequences of successful efforts to reduce sulfur in shipping fuel from 2020, as burning the dirtier fuel may have had a brightening effect on clouds. However, the accelerating energy budget imbalance began before this change. Natural fluctuations in the climate system such as the Pacific Decadal Oscillation might also be playing a role. Finally - and most worryingly - the cloud changes might be part of a trend caused by global warming itself, that is, a positive feedback on climate change. What does this mean? These findings suggest recent extremely hot years are not one-offs but may reflect a strengthening of warming over the coming decade or longer. This will mean a higher chance of more intense climate impacts from searing heatwaves, droughts and extreme rains on land, and more intense and long lasting marine heatwaves. This imbalance may lead to worse longer-term consequences. New research shows the only climate models coming close to simulating real world measurements are those with a higher "climate sensitivity". That means these models predict more severe warming beyond the next few decades in scenarios where emissions are not rapidly reduced. We don't know yet whether other factors are at play, however. It's still too early to definitively say we are on a high-sensitivity trajectory. Our eyes in the sky We've known the solution for a long time: stop the routine burning of fossil fuels and phase out human activities causing emissions such as deforestation. Keeping accurate records over long periods of time is essential if we are to spot unexpected changes. Satellites, in particular, are our advance warning system, telling us about heat storage changes roughly a decade before other methods. But funding cuts and drastic priority shifts in the United States may threaten essential satellite climate monitoring. (Author: Steven Sherwood, Professor of Atmospheric Sciences, Climate Change Research Centre, UNSW Sydney; Benoit Meyssignac, Associate Research Scientist in Climate Science, Université de Toulouse, and Thorsten Mauritsen, Professor of Climate Science, Stockholm University) (Disclaimer Statement: Steven Sherwood receives funding from the Australian Research Council and the Mindaroo Foundation. Benoit Meyssignac receives funding from the European Commission, the European Space Agency and the French National Space Agency. Thorsten Mauritsen receives funding from the European Research Council, the European Space Agency, the Swedish Research Council, the Swedish National Space Agency and the Bolin Centre for Climate Research.)

Scientists discover rare space alcohol that could explain how life began on the Earth
Scientists discover rare space alcohol that could explain how life began on the Earth

Time of India

time16 hours ago

  • Time of India

Scientists discover rare space alcohol that could explain how life began on the Earth

Astronomers have uncovered a cosmic clue that takes us closer to answering one of humanity's oldest questions, 'How did life begin on Earth?' It has been found out that a young star system, located roughly 330 light-years away, is awash in alcohol! The discovered alcohol types and their isotopes are among the building blocks of the starting points for creating even complex organic molecules like amino acids. Locating these bits in such a young planetary nursery suggests that the seeds of life might be spread throughout the galaxy, tied to how comets and icy materials form. An alcohol-soaked star system A discovery around the star HD 10045, which is about 330 light-years from Earth, has for the first time, allowed scientists to detect not only methanol, an alcohol compound, but also its rare isotopes in the protoplanetary disk encircling this young star. Published on June 5 in The Astrophysical Journal Letters, the research was based on data from the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile What makes these bits the 'cosmic alcohol'? Methanol is a simple alcohol that plays a crucial role in the formation of organic molecules like amino acids, the essential building blocks of life. Although methanol itself has been spotted in other star-forming disks, detecting its isotopes, which are also much rarer variants of the same, is an important step in the discovery of life's building block on Earth. As lead author Alice Booth from the Harvard & Smithsonian Center for Astrophysics explained, 'Finding these isotopes of methanol gives essential insight into the history of ingredients necessary to build life here on Earth.' by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like Rabien Ab: ten wysokiej klasy aparat słuchowy zdominuje rynek w 2025 roku DRUGIE UCHO Undo Why is HD 100453 different from the others? This star is about 1.6 times bigger than our Sun. Because it's larger, the disk of gas and dust around it is warmer. That warmth keeps methanol in gas form, even far from the star, making it much easier for telescopes like ALMA to detect. In contrast, stars smaller than our Sun have cooler disks, where methanol usually freezes into ice, making it much harder to spot. Another interesting factor about it is that the amount of methanol, as compared to other organic molecules in this star's disk, is very similar to what we see in comets from our own solar system. This gives scientists a clue that these icy materials might come together to form comets, which can then crash into young planets and deliver important ingredients for life. 'This research supports the idea that comets may have played a big role in delivering important organic material to the Earth billions of years ago,' said Milou Temmink, a PhD student who studies planet-forming disks at Leiden University A mix of space chemicals has life-building potential What scientists found goes beyond just simple methanol. The study suggests there may be even more complex molecules hiding in the gas around the star, including things that could be the early building blocks of amino acids and sugars, which are key ingredients for life. According to , these discoveries include rare types of methanol like ¹³CH₃OH and possibly deuterated methanol. Their presence means that icy materials floating in space might survive even during the wild, chaotic process of planet formation. What could it mean for life beyond Earth? By following these organic molecules, be it tiny ice grains, comets, or to planets, scientists are starting to connect the dots on how life might form in different parts of the universe. The chemical mix found around the star HD 100453 could be very similar to what helped spark life on Earth billions of years ago.

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into a world of global content with local flavor? Download Daily8 app today from your preferred app store and start exploring.
app-storeplay-store