activity
20102021
most citedSoft X-ray coronal spectra at low activity levels observed by RESIK

41 citations · 104 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2021

The Solar Line Emission Dopplerometer project

J. -M. Malherbe, P. Mein, F. Sayede +4

Observations of the dynamics of solar coronal structures are necessary to investigate space weather phenomena and global heating of the corona. The profiles of high temperature lin…

astro-ph.SR2012★ 25 cited

Sphinx measurements of the 2009 solar minimum x-ray emission

J. Sylwester, M. Kowalinski, S. Gburek +9

The SphinX X-ray spectrophotometer on the CORONAS-PHOTON spacecraft measured soft X-ray emission in the 1-15 keV energy range during the deep solar minimum of 2009 with a sensitivi…

astro-ph.SR2011★ 23 cited

High time resolution observations of solar H-alpha flares - II. Search for signatures of electron beam heating

K. Radziszewski, P. Rudawy, K. J. H. Phillips

Aims. The H-alpha emission of solar flare kernels and associated hard X-ray (HXR) emission often show similar time variations but their light curves are shifted in time by energy t…

astro-ph.SR2010★ 13 cited

Search for Rapid Changes in the Visible-Light Corona during the 21 June 2001 Total Solar Eclipse

P. Rudawy, K. J. H. Phillips, A. Buczylko +2

Some 8000 images obtained with the SECIS fast-frame CCD camera instrument located at Lusaka, Zambia, during the total eclipse of 21 June 2001 have been analyzed to search for short…

astro-ph.SR2010★ 2 cited

The SECIS instrument on the Lomnicky Peak Observatory

J. Ambroz, K. Radziszewski, P. Rudawy +2

Heating mechanisms of the solar corona will be investigated at the high-altitude solar observatory Lomnicky Peak of the Astronomical Institute of SAS (Slovakia) using its mid-size…

astro-ph.SR2010★ 41 cited

Soft X-ray coronal spectra at low activity levels observed by RESIK

B. Sylwester, J. Sylwester, K. J. H. Phillips

The quiet-Sun X-ray emission is important for deducing coronal heating mechanisms, but it has not been studied in detail since the Orbiting Solar Observatory (OSO) spacecraft era.…