Jump to content

Recommended Posts

Posted
Proba-2_sees_two_partial_eclipses_card_f Video: 00:00:23

ESA’s Proba-2 captured two partial solar eclipses on 25 October 2022.

A solar eclipse is caused by the movement of the Moon around Earth. Despite their much different sizes, due to their separation, the Moon appears to be about the same size as the significantly larger Sun in the sky. Occasionally, the Moon passes in front of the Sun, blocking its light, so that part of the Earth’s surface is in the Moon’s shadow. The line-up is not always perfect, and so not every eclipse is a total solar eclipse.

On 25 October only part of the Sun’s light was blocked by the Moon, creating what is known as a partial eclipse. It was visible from most of Europe, North-Africa, the middle East and parts of Asia, with the Moon blocking 82% of the sunlight near the North Pole. In Europe up to 40% of the sunlight was obscured during the event.

This partial eclipse was observed by ESA’s Proba-2 mission from its unique vantage point in space. Its SWAP instrument studies the Sun in the extreme ultraviolet (EUV) light where it focuses on the solar corona – the Sun’s hot turbulent atmosphere – at temperatures of about a million degrees. The corona is seen in the background of this video.

For us on Earth, the Moon passes only once in front of the Sun during a solar eclipse. Since Proba-2 orbits the Earth in about 100 minutes, it was able to observe this eclipse not once but twice. Additionally, the Moon was first observed while traversing the field of view in the upper right corner, but not blocking any solar light. The first observation of the eclipse around 10:30 UTC (12:30 CEST) was cut short as Proba-2 experienced an occultation. Such an occultation occurs when Proba-2 flies through the Earth’s atmosphere and the SWAP instrument is not active. The second partial eclipse was captured around 12:25 UTC (14:25 CEST). This movie shows both the eclipses.

ESA's Sun-watching spacecraft monitor the Sun's behaviour to better understand the influence of space weather on our home planet. The ESA-led Solar Orbiter mission, in partnership with NASA, is orbiting the Sun from closer than ever before and will provide the first high resolution images of the Sun's poles. Meanwhile ESA Vigil will be the first mission to keep a constant eye on brewing space weather events, to better protect vital infrastructure on Earth and in orbit. 

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

  • Similar Topics

    • By European Space Agency
      The second of the Meteosat Third Generation (MTG) satellites and the first instrument for the Copernicus Sentinel-4 mission are fully integrated and, having completed their functional and environmental tests, they are now ready to embark on their journey to the US for launch this summer.
      View the full article
    • By NASA
      Explore This Section Science Science Activation Eclipses to Auroras: Eclipse… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science   3 min read
      Eclipses to Auroras: Eclipse Ambassadors Experience Winter Field School in Alaska
      In 2023 and 2024, two eclipses crossed the United States, and the NASA Science Activation program’s Eclipse Ambassadors Off the Path project invited undergraduate students and amateur astronomers to join them as “NASA Partner Eclipse Ambassadors”. This opportunity to partner with NASA, provide solar viewing glasses, and share eclipse knowledge with underserved communities off the central paths involved:
      Partnering with an undergraduate/amateur astronomer Taking a 3-week cooperative course (~12 hours coursework) Engaging their communities with eclipse resources by reaching 200+ people These Eclipse Ambassador partnerships allowed participants to grow together as they learned new tools and techniques for explaining eclipses and engaging with the public, and Eclipse Ambassadors are recognized for their commitment to public engagement.
      In January 2025, the Eclipse Ambassadors Off the Path project held a week-long Heliophysics Winter Field School (WFS), a culminating Heliophysics Big Year experience for nine undergraduate and graduate Eclipse Ambassadors. The WFS exposed participants to career opportunities and field experience in heliophysics, citizen science, and space physics. The program included expert lectures on space physics, aurora, citizen science, and instrumentation, as well as hands-on learning opportunities with Poker Flat Rocket Range, the Museum of the North, aurora chases, and more. Students not only learned about heliophysics, they also actively participated in citizen science data collection using a variety of instruments, as well as the Aurorasaurus citizen science project app. Interactive panels on career paths helped prepare them to pursue relevant careers.
      One participant, Sophia, said, “This experience has only deepened my passion for heliophysics, science communication, and community engagement.” Another participant, Feras, reflected, “Nine brilliant students from across the country joined a week-long program at the University of Alaska Fairbanks’ (UAF) Geophysical Institute, where we attended multiple panels on solar and space physics, spoke to Athabaskan elders on their connection to the auroras, and visited the Poker Flat Research Range to observe the stunning northern lights.”
      This undertaking would not have been possible without the coordination, planning, leadership of many. Principal Investigators included Vivian White (Eclipse Ambassadors, Astronomical Society of the Pacific, ASP) and Dr. Elizabeth McDonald (Aurorasaurus, NASA GSFC). Other partners included Lynda McGilvary (Geophysical Institute at UAF), Jen Arseneau (UAF), Shanil Virani (ASP), Andréa Hughes (NASA), and Lindsay Glesener (University of Minnesota), as well as knowledge holders, students, and scientists.
      The Eclipse Ambassadors Off the Path project is supported by NASA under cooperative agreement award number 80NSS22M0007 and is part of NASA’s Science Activation Portfolio. To learn more, visit: www.eclipseambassadors.org.
      Winter Field School Participants standing under the aurora. Andy Witteman Share








      Details
      Last Updated Feb 18, 2025 Editor NASA Science Editorial Team Related Terms
      Science Activation 2023 Solar Eclipse 2024 Solar Eclipse Auroras Opportunities For Students to Get Involved Explore More
      2 min read An Afternoon of Family Science and Rocket Exploration in Alaska


      Article


      4 days ago
      3 min read Tribal Library Co-Design STEM Space Workshop


      Article


      5 days ago
      5 min read NASA Rockets to Fly Through Flickering, Vanishing Auroras


      Article


      4 weeks ago
      Keep Exploring Discover More Topics From NASA
      James Webb Space Telescope


      Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…


      Perseverance Rover


      This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial…


      Parker Solar Probe


      On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona…


      Juno


      NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to…

      View the full article
    • By European Space Agency
      On 13 and 14 February 2025, the European Space Agency (ESA) celebrated 20 years of supporting space innovation through its ESA Business Incubation Centres (BIC) network. The event in Munich, Germany, brought together entrepreneurs, successful space companies, experts and policymakers.
      View the full article
    • By European Space Agency
      Image: XMM-Newton finds two stray supernova remnants View the full article
    • By NASA
      3 min read
      NASA Solar Observatory Sees Coronal Loops Flicker Before Big Flares
      For decades, scientists have tried in vain to accurately predict solar flares — intense bursts of light on the Sun that can send a flurry of charged particles into the solar system. Now, using NASA’s Solar Dynamics Observatory, one team has identified flickering loops in the solar atmosphere, or corona, that seem to signal when the Sun is about to unleash a large flare.
      These warning signs could help NASA and other stakeholders protect astronauts as well as technology both in space and on the ground from hazardous space weather.
      NASA’s Solar Dynamics Observatory captured this image of coronal loops above an active region on the Sun in mid-January 2012. The image was taken in the 171 angstrom wavelength of extreme ultraviolet light. NASA/Solar Dynamics Observatory Led by heliophysicist Emily Mason of Predictive Sciences Inc. in San Diego, California, the team studied arch-like structures called coronal loops along the edge of the Sun. Coronal loops rise from magnetically driven active regions on the Sun, where solar flares also originate.
      The team looked at coronal loops near 50 strong solar flares, analyzing how their brightness in extreme ultraviolet light varied in the hours before a flare compared to loops above non-flaring regions. Like flashing warning lights, the loops above flaring regions varied much more than those above non-flaring regions.
      “We found that some of the extreme ultraviolet light above active regions flickers erratically for a few hours before a solar flare,” Mason explained. “The results are really important for understanding flares and may improve our ability to predict dangerous space weather.”
      Published in the Astrophysical Journal Letters in December 2024 and presented on Jan. 15, 2025, at a press conference during the 245th meeting of the American Astronomical Society, the results also hint that the flickering reaches a peak earlier for stronger flares. However, the team says more observations are needed to confirm this link.
      To view this video please enable JavaScript, and consider upgrading to a web browser that
      supports HTML5 video
      The four panels in this movie show brightness changes in coronal loops in four different wavelengths of extreme ultraviolet light (131, 171, 193, and 304 angstroms) before a solar flare in December 2011. The images were taken by the Atmospheric Imaging Assembly (AIA) on NASA’s Solar Dynamics Observatory and processed to reveal flickering in the coronal loops. NASA/Solar Dynamics Observatory/JHelioviewer/E. Mason Other researchers have tried to predict solar flares by examining magnetic fields on the Sun, or by looking for consistent trends in other coronal loop features. However, Mason and her colleagues believe that measuring the brightness variations in coronal loops could provide more precise warnings than those methods — signaling oncoming flares 2 to 6 hours ahead of time with 60 to 80 percent accuracy.
      “A lot of the predictive schemes that have been developed are still predicting the likelihood of flares in a given time period and not necessarily exact timing,” said team member Seth Garland of the Air Force Institute of Technology at Wright-Patterson Air Force Base in Ohio.
      Each solar flare is like a snowflake — every single flare is unique.
      Kara kniezewski
      Air Force Institute of Technology
      “The Sun’s corona is a dynamic environment, and each solar flare is like a snowflake — every single flare is unique,” said team member Kara Kniezewski, a graduate student at the Air Force Institute of Technology and lead author of the paper. “We find that searching for periods of ‘chaotic’ behavior in the coronal loop emission, rather than specific trends, provide a much more consistent metric and may also correlate with how strong a flare will be.”
      The scientists hope their findings about coronal loops can eventually be used to help keep astronauts, spacecraft, electrical grids, and other assets safe from the harmful radiation that accompanies solar flares. For example, an automated system could look for brightness changes in coronal loops in real-time images from the Solar Dynamics Observatory and issue alerts.
      “Previous work by other researchers reports some interesting prediction metrics,” said co-author Vadim Uritsky of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and the Catholic University of Washington in D.C. “We could build on this and come up with a well-tested and, ideally, simpler indicator ready for the leap from research to operations.”
      By Vanessa Thomas
      NASA’s Goddard Space Flight Center, Greenbelt, Md.
      Share








      Details
      Last Updated Jan 15, 2025 Related Terms
      Goddard Space Flight Center Heliophysics Heliophysics Division Space Weather The Sun Explore More
      7 min read NASA Celebrates Edwin Hubble’s Discovery of a New Universe


      Article


      5 hours ago
      6 min read NASA’s Webb Reveals Intricate Layers of Interstellar Dust, Gas


      Article


      1 day ago
      6 min read Newfound Galaxy Class May Indicate Early Black Hole Growth, Webb Finds


      Article


      1 day ago
      Keep Exploring Discover More Topics From NASA
      Missions



      Humans in Space



      Climate Change



      Solar System


      View the full article
  • Check out these Videos

×
×
  • Create New...