Year |
Citation |
Score |
2023 |
Grajeda JA, Boucheron LE, Kirk MS, Leisner A, Arge CN. Quantifying the Consistency and Characterizing the Confidence of Coronal Holes Detected by Active Contours Without Edges (ACWE). Solar Physics. 298: 133. PMID 38028404 DOI: 10.1007/s11207-023-02228-0 |
0.312 |
|
2019 |
Jess DB, Dillon CJ, Kirk MS, Reale F, Mathioudakis M, Grant SDT, Christian DJ, Keys PH, Prasad SK, Houston SJ. Statistical Signatures of Nanoflare Activity. I. Monte Carlo Simulations and Parameter-space Exploration The Astrophysical Journal. 871: 133. DOI: 10.3847/1538-4357/Aaf8Ae |
0.438 |
|
2017 |
Kirk MS, Balasubramaniam KS, Jackiewicz J, Gilbert HR. The Origin of Sequential Chromospheric Brightenings Solar Physics. 292: 72. DOI: 10.1007/S11207-017-1094-3 |
0.609 |
|
2015 |
Mumford SJ, Christe S, Pérez-Suárez D, Ireland J, Shih AY, Inglis AR, Liedtke S, Hewett RJ, Mayer F, Hughitt K, Freij N, Meszaros T, Bennett SM, Malocha M, Evans J, ... ... Kirk MS, et al. SunPy - Python for solar physics Computational Science and Discovery. 8. DOI: 10.1088/1749-4699/8/1/014009 |
0.393 |
|
2014 |
Kirk MS, Balasubramaniam KS, Jackiewicz J, James McAteer RT. Qualities of sequential chromospheric brightenings observed in Hα and UV images Astrophysical Journal. 796. DOI: 10.1088/0004-637X/796/2/78 |
0.599 |
|
2014 |
Hess Webber SA, Karna N, Pesnell WD, Kirk MS. Areas of Polar Coronal Holes from 1996 Through 2010 Solar Physics. DOI: 10.1007/S11207-014-0564-0 |
0.439 |
|
2013 |
Kirk MS, Balasubramaniam KS, Jackiewicz J, McNamara BJ, McAteer RTJ. An Automated Algorithm to Distinguish and Characterize Solar Flares and Associated Sequential Chromospheric Brightenings Solar Physics. 283: 97-111. DOI: 10.1007/S11207-011-9843-1 |
0.607 |
|
2012 |
Kirk MS, Balasubramaniam KS, Jackiewicz J, McAteer RTJ, Milligan RO. Properties of sequential chromospheric brightenings and associated flare ribbons Astrophysical Journal. 750. DOI: 10.1088/0004-637X/750/2/145 |
0.619 |
|
2009 |
Kirk MS, Pesnell WD, Young CA, Hess Webber SA. Automated detection of EUV polar coronal holes during solar cycle 23 Solar Physics. 257: 99-112. DOI: 10.1007/S11207-009-9369-Y |
0.391 |
|
Show low-probability matches. |