Year |
Citation |
Score |
2020 |
Kallunki J, Tornikoski M, Björklund I. Identifying 8 mm Radio Brightenings During the Solar Activity Minimum Solar Physics. 295: 105. DOI: 10.1007/S11207-020-01673-5 |
0.509 |
|
2020 |
Kallunki J, Tornikoski M, Kirves P, Oinaskallio E, Aatrokoski J, Mujunen A, Tammi J. Solar polarization observations at 3 and 13 mm Astronomische Nachrichten. 341: 118-124. DOI: 10.1002/Asna.202013684 |
0.368 |
|
2019 |
Selhorst CL, Kallunki J, Castro CGGd, Valio A, Costa JER. The Solar Radius at 37 GHz through Cycles 22 to 24 Solar Physics. 294: 175. DOI: 10.1007/S11207-019-1568-6 |
0.513 |
|
2018 |
Kallunki J, Tornikoski M. Measurements of the Quiet-Sun Level Brightness Temperature at 8 mm Solar Physics. 293: 156. DOI: 10.1007/S11207-018-1380-8 |
0.364 |
|
2018 |
Kallunki J, Tornikoski M, Oinaskallio E, Kirves P, Aatrokoski J, Mujunen A, Tammi J. Solar observing system for radio frequencies 5–120 MHz Astronomische Nachrichten. 339: 656-660. DOI: 10.1002/Asna.201913545 |
0.454 |
|
2018 |
Kallunki J, Tornikoski M, Tammi J, Kinnunen E, Korhonen K, Kesäläinen S, Arkko O. Forty years of solar radio observations at Metsähovi Radio Observatory Astronomische Nachrichten. 339: 204-211. DOI: 10.1002/Asna.201813464 |
0.491 |
|
2017 |
Hodgson JA, Krichbaum TP, Marscher AP, Jorstad SG, Rani B, Marti-Vidal I, Bach U, Sanchez S, Bremer M, Lindqvist M, Uunila M, Kallunki J, Vicente P, Fuhrmann L, Angelakis E, et al. Location of γ-ray emission and magnetic field strengths in OJ 287 Astronomy and Astrophysics. 597: 80. DOI: 10.1051/0004-6361/201526727 |
0.367 |
|
2017 |
Kallunki J, Tornikoski M. Eruptive Solar Prominence at 37 GHz Solar Physics. 292: 84. DOI: 10.1007/S11207-017-1110-7 |
0.472 |
|
2017 |
Kallunki J, Uunila M. Sizes of solar active regions at 8 mm Astronomische Nachrichten. 338: 398-406. DOI: 10.1002/Asna.201613196 |
0.345 |
|
2016 |
Duev DA, Pogrebenko SV, Cimò G, Molera Calvés G, Bocanegra Bahamón TM, Gurvits LI, Kettenis MM, Kania J, Tudose V, Rosenblatt P, Marty JC, Lainey V, De Vicente P, Quick J, Nickola M, ... ... Kallunki J, et al. Planetary Radio Interferometry and Doppler Experiment (PRIDE) technique: A test case of the Mars Express Phobos fly-by Astronomy and Astrophysics. 593. DOI: 10.1051/0004-6361/201628869 |
0.317 |
|
2015 |
Uunila M, Kallunki J. Reliability of 1.8-meter solar radio telescope at Metsähovi Radio Observatory for long-term solar monitoring Astrophysics and Space Science. 359: 33. DOI: 10.1007/S10509-015-2481-6 |
0.527 |
|
2015 |
Smirnova VV, Riehokainen A, Solov’ev AA, Kallunki J. Time delay effect between long quasi-periodic oscillations of 37 GHz radio sources and the magnetic field of the nearest sunspots Astrophysics and Space Science. 357: 149. DOI: 10.1007/S10509-015-2382-8 |
0.432 |
|
2015 |
Kallunki J, Uunila M, McKay-Bukowski D. Multi-frequency solar observations at Metsähovi Radio Observatory and KAIRA Astronomische Nachrichten. 336: 566-569. DOI: 10.1002/Asna.201512194 |
0.555 |
|
2014 |
Molera Calvés G, Pogrebenko SV, Cimò G, Duev DA, Bocanegra-Bahamón TM, Wagner JF, Kallunki J, De Vicente P, Kronschnabl G, Haas R, Quick J, MacCaferri G, Colucci G, Wang WH, Yang WJ, et al. Observations and analysis of phase scintillation of spacecraft signal on the interplanetary plasma Astronomy and Astrophysics. 564. DOI: 10.1051/0004-6361/201322925 |
0.432 |
|
2012 |
Kallunki J, Riehokainen A. Investigation of Quasi-periodic Solar Oscillations in Sunspots Based on SOHO/MDI Magnetograms Solar Physics. 280: 347-354. DOI: 10.1007/S11207-012-0021-X |
0.436 |
|
2012 |
Kallunki J, Pohjolainen S. Radio Pulsating Structures with Coronal Loop Contraction Solar Physics. 280: 491-507. DOI: 10.1007/S11207-012-0003-Z |
0.378 |
|
2012 |
Kallunki J, Riehokainen A. The statistical study of quasi-periodic oscillations of the radio emission in solar quiet regions Astronomische Nachrichten. 333: 20-25. DOI: 10.1002/Asna.201111630 |
0.495 |
|
2011 |
Smirnova V, Riehokainen A, Ryzhov V, Zhiltsov A, Kallunki J. Long-period oscillations of millimeter emission above sunspots Astronomy and Astrophysics. 534. DOI: 10.1051/0004-6361/201117483 |
0.449 |
|
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