RUS ↔ ENG

About the project

The Laboratory of X-Ray Astronomy of the Sun is a subdivision of the Spectroscopy department in the Lebedev Institute of the Russian Academy of Science. The laboratory was founded during the end of the 1970s, with the aim of studying the Sun and other space objects from rockets and spacecrafts.

Research of the Sun was started in the institute in 1947th onboard rockets R1a and, with the beginning of the space era, were continued using the artificial Earth satellites. In 1957, the scientist of Lebedev Institute for the first time observed short wavelength emission of the Sun from onboard of the second Russian satellite ("Sputnik-2"). In 1963, the first X-ray image of the Sun was obtained. At the end of the 1960s, the first X-ray spectra with the wavelength shorter than 10 angstrom were registered.

Today the laboratory is the leading Russian center to design and construct space telescopes for solar researches. The instruments created in the laboratory operated onboard several "Intercosmos" satellites, onboard interplanetary Fobos stations, and onboard three spacecrafts launched in the frameworks of the CORONAS space program. Now the laboratory is working on developing four scientific instruments intended for the Russian space mission "Interhelioprobe." The laboratory team is also responsible for the "ARKA" project - unique solar telescopes that will provide for the first time the images of solar corona with a spatial resolution of about 100 km. The laboratory also participates in several other projects.

The laboratory has approximately 30 staff members.

project diary

Another beautiful flare on the far side of the Sun
The video shows a rather spectacular solar event that occurred overnight between Tuesday and Wednesday. The flare took place on the far side of the Sun and was classified as an M5 event (approximately 50% of the intensity of the strongest X-class flares).
The decline in solar activity continues
Solar activity continues to decline. Solar X-ray flux, which remained near the M-class level early in the week, has dropped tenfold over the past four days and is currently below the C-class level. The geomagnetic storm forecast is also green.
Diary's archive

Astronomy news

NASA's Spitzer Images Out-of-This-World Galaxy
NASA's Spitzer Space Telescope has imaged a wild creature of the dark -- a coiled galaxy with an eye-like object at its center.
Saturnian Moon Shows Evidence Of Ammonia
Data collected during two close flybys of Saturn's moon Enceladus by NASA's Cassini spacecraft add more fuel to the fire about the Saturnian ice world containing sub-surface liquid water. The data collected by Cassini's Ion and Neutral Mass Spectrometer during Enceladus flybys in July and Oct. 2008, were released in the July 23 issue of the journal Nature.
Double Engine Fuels Star's Remarkable Nebula
ESO has just released a stunning new image of a field of stars towards the constellation of Carina (the Keel). This striking view is ablaze with a flurry of stars of all colors and brightnesses, some of which are seen against a backdrop of clouds of dust and gas. One unusual star in the middle, HD 87643, has been extensively studied with several ESO telescopes, including the Very Large Telescope Interferometer (VLTI)
News archive

Space weather

Magnetic storms in the last 24 hours:

No geomagnetic storms were observed

Magnetic storms

Magnetic storms in the next 24 hours:

are not expected

Magnetic storm forecast

Current activity of the Sun:

Solar radio flux (10.7 cm) = 101
Mean planetary A index = 4
Mean planetary Kp index =
Solar flares today

The Sun today

Solar chromosphere today

Solar chromosphere

Solar photosphere today

Solar photosphere

(Sun in the visible rays)
Transition region today

Transition region

The Solar corona today

The Solar corona

click image to view

View all Solar images

Sunspot groups

Sunspot groups

The following regions with sunspots can be now observed on the Sun's surface:
  • NOAA 4491 - coordinates S11 E54
  • NOAA 4489 - coordinates S07 E17
  • NOAA 4482 - coordinates S09 W93

Solar flocculi

The following H-alpha plages without spots can be currently observed on the Sun's surface:
  • NOAA 4490 - coordinates N15 E07
  • NOAA 4488 - coordinates N23 W91
  • NOAA 4487 - coordinates N08 W92
Sunspots in more detail