Asian Surveying & Mapping
Breaking News
HAL to build, market Isro’s SSLV in landmark deal
New Delhi, Jun 20: In a historic move for...
Taiwan developing space capabilities for all-weather imaging
TAIPEI (TVBS News) — Taiwan is advancing its space...
Honda hails successful test of reusable rocket as it looks to get into the space business
Tokyo — Japan's second-biggest carmaker, Honda, has successfully tested...
China’s space program provides larger platform for broader international cooperation
BEIJING -- Experts from China's manned space program said...
India To Launch $1.5 Billion Joint Earth Mission With NASA In July
National Aeronautics and Space Administration (NASA) and the Indian...
Axiom-4 mission delayed again: ISRO confirms Subhanshu Shukla’s ISS spaceflight won’t launch before 22 June 2025
The Axiom-4 mission to the International Space Station has...
Mengzhou spacecraft for China’s moon-landing mission passes landmark test flight
China has completed the inaugural test flight of its...
Space application for ITMA Asia + CITME 2026 opens
Shanghai – Space application for the 2026 edition of...
Yanmar, Chia Tai and XAG Empower Thai Agriculture through Innovation
Bang Nam Priao District, Chachoengsao Province, Thailand – On...
bitsensing Signs MOU with IKIO Technologies to Advance AI-Based Traffic Monitoring on India’s Expressways, Highways and Municipal Areas
Backed by proven success in South Korea and Europe,...
Although solar energy sources are located at the core of the Sun, the temperature of the upper part of the solar atmosphere (i.e., chromosphere and corona) is higher than that of the visible surface (i.e., photosphere). The mechanisms that produce such a peculiar behavior are still a mystery for solar researchers.

A Japanese research team tried to tackle this for the first time, evaluating how much energy is dissipated at the chromosphere through waves. Results show that the amount of dissipated energy is 10 times larger than the required energy to maintain the chromosphere. Therefore, waves could be responsible for heating the upper chromosphere up to its present values (i.e., 10,000 Kelvin).

This discovery was found thanks to an international collaboration among Japanese and U.S. solar-observing satellites. The Hinode mission revealed tiny fluctuations of physical parameters through spectropolarimetric observations, and the IRIS (Interface Region Imaging Spectrograph) performed spectroscopic observations to derive physical information of the upper chromosphere. The combination of these satellites made it possible to evaluate dissipated energy by comparing the energy fluxes obtained at the two atmospheric layers.

Hinode and IRIS satellites helped discover that the dynamic solar chromosphere could be heated and formed by dissipation of energy of waves. (Credit:  NAOJ/JAXA)

Hinode and IRIS satellites helped discover that the dynamic solar chromosphere could be heated and formed by dissipation of energy of waves. (Credit: NAOJ/JAXA)