Add to ORKGLocalized increase of the magnetic field observed by routine methods on the photosphere result in th...
The Very Large Array (VLA) and the Westerbork Synthesis Radio Telescope (WSRT) were used for making ...
The sudden release of magnetic energy on the Sun drives powerful solar flares and coronal mass eject...
Characteristics of solar active regions responsible for generation of type 3 radio bursts at hectome...
Active heliographic longitudes at the sun are investigated by using the observational data for long-...
Comparison of satellite interplanetary magnetic field observations with photospheric magnetic field ...
The synoptic appearance of solar magnetic sectors is studied using 454 sector boundaries observed at...
Observations related to large-scale structure of interplanetary magnetic field, solar origin, and ge...
Solar surface and interplanetary magnetic fields, interplanetary plasmas, and geomagnetic field sola...
The solar radio sweep-frequency observations and hours of patrol from five rad radio observatories f...
The following efforts were completed in support of the Solar Maximum Mission (SMM): (1) the evolutio...
Chree (superposed epoch) analyses of Jupiter's decameter-wave radio emission taken from the new Thie...
The interplanetary magnetic field near 1 AU has a characteristic “sector” structure that reflects it...
This brief history is organized around the long problem of the solar M region, i.e. the structure on...
Interplanetary magnetic field measured by Pioneer 8 during solar event of 25 Feb. 196
Localized increase of the magnetic field observed by routine methods on the photosphere result in th...
The Very Large Array (VLA) and the Westerbork Synthesis Radio Telescope (WSRT) were used for making ...
The sudden release of magnetic energy on the Sun drives powerful solar flares and coronal mass eject...
Characteristics of solar active regions responsible for generation of type 3 radio bursts at hectome...
Active heliographic longitudes at the sun are investigated by using the observational data for long-...
Comparison of satellite interplanetary magnetic field observations with photospheric magnetic field ...
The synoptic appearance of solar magnetic sectors is studied using 454 sector boundaries observed at...
Observations related to large-scale structure of interplanetary magnetic field, solar origin, and ge...
Solar surface and interplanetary magnetic fields, interplanetary plasmas, and geomagnetic field sola...
The solar radio sweep-frequency observations and hours of patrol from five rad radio observatories f...
The following efforts were completed in support of the Solar Maximum Mission (SMM): (1) the evolutio...
Chree (superposed epoch) analyses of Jupiter's decameter-wave radio emission taken from the new Thie...
The interplanetary magnetic field near 1 AU has a characteristic “sector” structure that reflects it...
This brief history is organized around the long problem of the solar M region, i.e. the structure on...
Interplanetary magnetic field measured by Pioneer 8 during solar event of 25 Feb. 196
Localized increase of the magnetic field observed by routine methods on the photosphere result in th...
The Very Large Array (VLA) and the Westerbork Synthesis Radio Telescope (WSRT) were used for making ...
The sudden release of magnetic energy on the Sun drives powerful solar flares and coronal mass eject...