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| 001 | 315521 | ||
| 005 | 20211110140137.0 | ||
| 020 | _ | _ | |a 978-3-935702-59-1 |
| 024 | 7 | _ | |a 10.3204/DESY-PROC-2014-03/chowdhury_partha |2 datacite_doi |
| 024 | 7 | _ | |a 1435-8077 |2 ISSN |
| 037 | _ | _ | |a PUBDB-2016-05928 |
| 100 | 1 | _ | |a Chowdhury, Partha |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 10th Patras Workshop on Axions, WIMPs and WISPs |c Geneva |d 2014-06-29 - 2014-07-04 |g AXION-WIMP 2014 |0 C14-06-29.1 |2 inspire |w Switzerland |
| 245 | _ | _ | |a Periodicities in the soft X-ray emission from the solar corona during descending phase of cycle 23 |
| 260 | _ | _ | |a Hamburg |c 2014 |b Verlag Deutsches Elektronen-Synchrotron |
| 295 | 1 | 0 | |a Chowdhury, Partha "Periodicities in the soft X-ray emission from the solar corona during descending phase of cycle 23" in Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 : 10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29 - 2014-07-04, Geneva |
| 300 | _ | _ | |a 141-146 |
| 336 | 7 | _ | |a CONFERENCE_PAPER |2 ORCID |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
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| 490 | 0 | _ | |a DESY-PROC |0 PERI:(DE-600)2450075-6 |
| 520 | _ | _ | |a We have studied the time series of full disk integrated soft X-ray emission from the solar corona during January 2004 to December 2008, covering the entire descending phase of solar cycle 23 from a global point of view. We employ the daily X-ray index (DXI) derived from 1s cadence X-ray observations from the Si detector of ``Solar X-ray Spectrometer (SOXS)'' mission in four different energy bands ranging between $6 - 25~KeV$. The daily time series is subjected to power spectrum analysis after appropriate correction for noise. Lomb-Scargle periodogram technique has shown prominent periods of $ \sim13.5$ days, $ \sim 27$ days, and near Rieger period of $ \sim 181$ days and $ \sim 1.24$ years in all energy bands. Further to this, other periods like $ \sim 31$, $\sim 48$, $\sim 57$, $\sim 76$, $\sim 96$, $\sim 130$, $\sim 227$ and $\sim 303$ days are also detected in different energy bands. We discuss our results in the light of previous observations and existing numerical models. |
| 787 | 0 | _ | |a Tsesmelis, Emmanuel et. al. |d Verlag Deutsches Elektronen-Synchrotron |i isPartOf |0 PUBDB-2016-05897 |r DESY-PROC-2014-03 |t Proceedings, 10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2014) : Geneva, Switzerland, June 29-July 4, 2014 |
| 856 | 4 | _ | |u https://bib-pubdb1.desy.de/record/315521/files/fulltext.pdf |y OpenAccess |
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| 910 | 1 | _ | |a University College of Science \ and Technology - Calcutta University - Kolkata 700009 - West Bengal - India |0 I:(DE-HGF)0 |b 0 |6 P:(DE-HGF)0 |
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