參考文獻 |
[1] Alissandrakis, C. E., Nindos, A., Patsourakos, S., & Hillaris, A. 2021, Multiwavelength observations of a metric type-II event, Astronomy and Astrophysics, 654, A112. https://doi.org/10.1051/0004-6361/202141672
[2] Alissandrakis, C. E., Nindos, A., Patsourakos, S., Kontogeorgos, A., & Tsitsipis, P. 2015, A tiny event producing an interplanetary type III burst, Astronomy & Astrophysics, 582. https://doi.org/10.1051/0004-6361/201526265
[3] Alvarez, H., & Haddock, F. T. 1973a, Decay time of type III solar bursts observed at kilometric wavelengths, Solar Physics, 30, 175. https://doi.org/10.1007/BF00156186
[4] Alvarez, H., & Haddock, F. T. 1973b, Solar Wind Density Model from km-Wave Type III Bursts, Solar Physics, 29, 197. https://doi.org/10.1007/bf00153449
[5] Aschwanden, M. J. 2005, in Physics of the Solar Corona: An Introduction with Problems and Solutions, ed. M. J. Aschwanden (Berlin, Heidelberg: Springer Berlin Heidelberg), 637
[6] Aschwanden, M. J., Benz, A. O., & Montello, M. L. 1994, Coherent-Phase or Random-Phase Acceleration of Electron Beams in Solar Flares, The Astrophysical Journal, 431, 432. https://doi.org/10.1086/174497
[7] Aubier, M. G., Leblanc, Y., & Moller-Pedersen, B. 1978, Type I and Type Ill Storm Radiation, Astronomy and Astrophysics, 70, 685.
[8] Badman, S. T., et al. 2022, Tracking a Beam of Electrons from the Low Solar Corona into Interplanetary Space with the Low Frequency Array, Parker Solar Probe, and 1 au Spacecraft, The Astrophysical Journal, 938, 95. https://doi.org/10.3847/1538-4357/ac90c2
[9] Bale, S. D., et al. 2016, The FIELDS Instrument Suite for Solar Probe Plus. Measuring the Coronal Plasma and Magnetic Field, Plasma Waves and Turbulence, and Radio Signatures of Solar Transients, Space Science Reviews, 204, 49. https://doi.org/10.1007/s11214-016-0244-5
[10] Benz, A. O. 2002, Plasma astrophysics [electronic resource] : kinetic processes in solar and stellar coronae / by Arnold O. Benz (2nd ed.; Dordrecht ;: Kluwer Academic Publishers)
[11] Benz, A. O., Monstein, C., & Meyer, H. 2005, Callisto A New Concept for Solar Radio Spectrometers, Solar Physics, 226, 143. https://doi.org/10.1007/s11207-005-5688-9
[12] Boischot, A., de La Noe, J., & Moller-Pedersen, B. 1970, Relation between Metric and Decametric Noise Storm Activity, Astronomy and Astrophysics, 4, 159.
[13] Bougeret, J.-L., Fainberg, J., & Stone, R. G. 1984, Interplanetary radio storms. II - Emission levels and solar wind speed in the range 0.05-0.8 AU, Astronomy and Astrophysics, 141, 17.
[14] Bougeret, J.-L., et al. 1998, A shock associated (SA) radio event and related phenomena observed from the base of the solar corona to 1 AU, Geophysical Research Letters, 25, 2513. https://doi.org/10.1029/98gl50563
[15] Bougeret, J. L., et al. 2008, S/WAVES: The Radio and Plasma Wave Investigation on the STEREO Mission, Space Science Reviews, 136, 487. https://doi.org/10.1007/s11214-007-9298-8
[16] Brueckner, G. E., et al. 1995, The Large Angle Spectroscopic Coronagraph (LASCO), Solar Physics, 162, 357. https://doi.org/10.1007/bf00733434
[17] Cairns, I. H., Robinson, P. A., & Zank, G. P. 2000, Progress on Coronal, Interplanetary, Foreshock, and Outer Heliospheric Radio Emissions, Publications of the Astronomical Society of Australia, 17, 22. https://doi.org/10.1071/AS00022
[18] Cane, H. V., Stone, R. G., Fainberg, J., Stewart, R. T., Steinberg, J. L., & Hoang, S. 1981, Radio evidence for shock acceleration of electrons in the solar corona, Geophysical Research Letters, 8, 1285. https://doi.org/10.1029/GL008i012p01285
[19] Cattell, C., et al. 2021, Periodicities in an active region correlated with Type III radio bursts observed by Parker Solar Probe, Astronomy and Astrophysics, 650, A6. https://doi.org/10.1051/0004-6361/202039510
[20] Cerruti, A. P., Kintner, P. M., Gary, D. E., Mannucci, A. J., Meyer, R. F., Doherty, P., & Coster, A. J. 2008, Effect of intense December 2006 solar radio bursts on GPS receivers, Space Weather, 6, n/a. https://doi.org/10.1029/2007sw000375
[21] Chen, L., Ma, B., Wu, D., Zhao, G., Tang, J., & Bale, S. D. 2021, An Interplanetary Type IIIb Radio Burst Observed by Parker Solar Probe and Its Emission Mechanism, The Astrophysical Journal, 915, L22. https://doi.org/10.3847/2041-8213/ac0b43
[22] Chree, C. 1913, Some Phenomena of Sunspots and of Terrestrial Magnetism at Kew Observatory, Philosophical Transactions of the Royal Society of London Series A, 212, 75. https://doi.org/10.1098/rsta.1913.0003
[23] Culhane, J. L., et al. 2007, The EUV Imaging Spectrometer for Hinode, Solar Physics, 243, 19. https://doi.org/10.1007/s01007-007-0293-1
[24] Del Zanna, G., Aulanier, G., Klein, K.-L., & Török, T. 2011, A single picture for solar coronal outflows and radio noise storms, Astronomy and Astrophysics, 526, A137. https://doi.org/10.1051/0004-6361/201015231
[25] Domingo, V., Fleck, B., & Poland, A. I. 1995, The SOHO Mission: an Overview, Solar Physics, 162, 1. https://doi.org/10.1007/bf00733425
[26] Dulk, G. A. 1990, Interplanetary Particle Beams, Solar Physics, 130, 139. https://doi.org/10.1007/bf00156785
[27] Dulk, G. A., & Marsh, K. A. 1982, Simplified expressions for the gyrosynchrotron radiation from mildly relativistic, nonthermal and thermal electrons, The Astrophysical Journal, 259, 350. https://doi.org/10.1086/160171
[28] Dulk, G. A., & Suzuki, S. 1980, The position and polarization of Type III solar bursts, Astronomy and Astrophysics, 88, 203.
[29] Evans, L. G., Fainberg, J., & Stone, R. G. 1973, Characteristics of Type III Exciters Derived from Low Frequency Radio Observations, Solar Physics, 31, 501. https://doi.org/10.1007/bf00152825
[30] Fainberg, J., & Stone, R. G. 1970, Type III Solar Radio Burst Storms Observed at Low Frequencies, Solar Physics, 15, 222. https://doi.org/10.1007/bf00149487
[31] Fox, N. J., et al. 2016, The Solar Probe Plus Mission: Humanity′s First Visit to Our Star, Space Science Reviews, 204, 7. https://doi.org/10.1007/s11214-015-0211-6
[32] Fränz, M., & Harper, D. 2002, Heliospheric coordinate systems, Planetary and Space Science, 50, 217. https://doi.org/10.1016/s0032-0633(01)00119-2
[33] Gary, D. E., & Hurford, G. J. 1989, Solar radio burst spectral observations, particle acceleration, and wave-particle interactions, Washington DC American Geophysical Union Geophysical Monograph Series, 54, 237. https://doi.org/10.1029/GM054p0237
[34] Gary, D. E., & Hurford, G. J. 2005, in Solar and Space Weather Radiophysics: Current Status and Future Developments, eds. D. E. Gary, & C. U. Keller (Dordrecht: Springer Netherlands), 71
[35] Gieseler, J., et al. 2023, Solar-MACH: An open-source tool to analyze solar magnetic connection configurations, Frontiers in Astronomy and Space Sciences, 9. https://doi.org/10.3389/fspas.2022.1058810
[36] Gopalswamy, N. 2004. in Astrophysics and Space Science Library, Interplanetary Radio Bursts, eds. D. E. Gary, & C. U. Keller, 305
[37] Gopalswamy, N., et al. 2000, Radio-rich solar eruptive events, Geophysical Research Letters, 27, 1427. https://doi.org/10.1029/1999gl003665
[38] Harra, L., et al. 2021, The active region source of a type III radio storm observed by Parker Solar Probe during encounter 2, Astronomy and Astrophysics, 650, A7. https://doi.org/10.1051/0004-6361/202039514
[39] Hartz, T. R. 1964, Solar noise observations from the Alouette satellite, Annales d′Astrophysique, 27, 831.
[40] Hey, J. S. 1946, Solar Radiations in the 4–6 Metre Radio Wave-Length Band, Nature, 157, 47. https://doi.org/10.1038/157047b0
[41] Howard, R. A., et al. 2008, Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI), Space Science Reviews, 136, 67. https://doi.org/10.1007/s11214-008-9341-4
[42] Jansky, K. G. 1933, Radio Waves from Outside the Solar System, Nature, 132, 66. https://doi.org/10.1038/132066a0
[43] Kamide, Y., & Chian, A. C.-L. 2007, Handbook of the Solar-Terrestrial Environment
[44] Kasper, J. C., et al. 2016, Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus, Space Science Reviews, 204, 131. https://doi.org/10.1007/s11214-015-0206-3
[45] Kim, E.-H., Cairns, I. H., & Robinson, P. A. 2007, Extraordinary-Mode Radiation Produced by Linear-Mode Conversion of Langmuir Waves, Physical Review Letters, 99, 015003. https://doi.org/10.1103/PhysRevLett.99.015003
[46] Kirk, J. G., Melrose, D. B., Melrose, D. B., Priest, E. R., Benz, A. O., Courvoisier, T., & Astronomie, S. G. f. A. u. 1994, Plasma Astrophysics (Springer-Verlag)
[47] Kontar, E. P., et al. 2017, Imaging spectroscopy of solar radio burst fine structures, Nature Communications, 8, 1515. https://doi.org/10.1038/s41467-017-01307-8
[48] Krucker, S., Kontar, E. P., Christe, S., Glesener, L., & Lin, R. P. 2011, Electron Acceleration Associated with Solar Jets, The Astrophysical Journal, 742, 82. https://doi.org/10.1088/0004-637x/742/2/82
[49] Krupar, V., et al. 2018, Interplanetary Type III Bursts and Electron Density Fluctuations in the Solar Wind, The Astrophysical Journal, 857, 82. https://doi.org/10.3847/1538-4357/aab60f
[50] Krupar, V., et al. 2014, Statistical Survey of Type III Radio Bursts at Long Wavelengths Observed by the Solar TErrestrial RElations Observatory (STEREO)/ Waves Instruments: Radio Flux Density Variations with Frequency, Solar Physics, 289, 3121. https://doi.org/10.1007/s11207-014-0522-x
[51] Krupar, V., et al. 2020, Density Fluctuations in the Solar Wind Based on Type III Radio Bursts Observed by Parker Solar Probe, The Astrophysical Journal Supplement Series, 246. https://doi.org/10.3847/1538-4365/ab65bd
[52] Kundu, M. R. 1965, Solar radio astronomy (New York: Interscience Publication)
[53] Larosa, A., et al. 2022, Langmuir-Slow Extraordinary Mode Magnetic Signature Observations with Parker Solar Probe, The Astrophysical Journal, 927, 95. https://doi.org/10.3847/1538-4357/ac4e85
[54] Leblanc, Y., Dulk, G. A., & Hoang, S. 1995, The low radio frequency limit of solar type III bursts: Ulysses observations in and out of the ecliptic, Geophysical Research Letters, 22, 3429. https://doi.org/10.1029/95gl01717
[55] Leblanc, Y., Dulk, G. A., Hoang, S., Bougeret, J.-L., & Robinson, P. A. 1996, Type III radio bursts observed by ULYSSES pole to pole, and simultaneously by wind, Astronomy and Astrophysics, 316, 406.
[56] Lecacheux, A. 2011. in Planetary, Solar and Heliospheric Radio Emissions (PRE VII), Direction Finding and Polarization Measurements of SKR, eds. H. O. Rucker, W. S. Kurth, P. Louarn, & G. Fischer, 13
[57] Lemen, J. R., et al. 2012, The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO), Solar Physics, 275, 17. https://doi.org/10.1007/s11207-011-9776-8
[58] Leske, R. A., et al. 2020, Observations of the 2019 April 4 Solar Energetic Particle Event at the Parker Solar Probe, The Astrophysical Journal Supplement Series, 246, 35. https://doi.org/10.3847/1538-4365/ab5712
[59] Lodge, O. 1900, Signalling Across Space Without Wires: Being a Description of the Work of Hertz & His Successors (United Kingdom: "The Electrician" Printing and Publishing Company)
[60] Ma, B., Chen, L., Wu, D., Pulupa, M., & Bale, S. D. 2022, Discrepancy between the Low-frequency Cutoffs of Type III Radio Bursts Based on Simultaneous Observations by WIND and PSP, The Astrophysical Journal Letters, 932, L26. https://doi.org/10.3847/2041-8213/ac7525
[61] Ma, Y., Xie, R.-x., Zheng, X.-m., Wang, M., & Yi-hua, Y. 2012, A Statistical Analysis of the Type-III Bursts in Centimeter and Decimeter Wavebands, Chinese Astronomy and Astrophysics, 36, 175. https://doi.org/10.1016/j.chinastron.2012.04.008
[62] Mann, G., Jansen, F., MacDowall, R. J., Kaiser, M. L., & Stone, R. G. 1999, A heliospheric density model and type III radio bursts, Astronomy and Astrophysics, 348, 614.
[63] McCauley, P. I., Cairns, I. H., White, S. M., Mondal, S., Lenc, E., Morgan, J., & Oberoi, D. 2019, The Low-Frequency Solar Corona in Circular Polarization, Solar Physics, 294, 106. https://doi.org/10.1007/s11207-019-1502-y
[64] McComas, D. J., et al. 2016, Integrated Science Investigation of the Sun (ISIS): Design of the Energetic Particle Investigation, Space Science Reviews, 204, 187. https://doi.org/10.1007/s11214-014-0059-1
[65] Melrose, D. B. 2006, Depolarization of Radio Bursts Due to Reflection off Sharp Boundaries in the Solar Corona, The Astrophysical Journal, 637, 1113. https://doi.org/10.1086/498499
[66] Melrose, D. B. 2017, Coherent emission mechanisms in astrophysical plasmas, Reviews of Modern Plasma Physics, 1, 5. https://doi.org/10.1007/s41614-017-0007-0
[67] Mitchell, J. G., et al. 2020, Small Electron Events Observed by Parker Solar Probe/IS⊙IS during Encounter 2, The Astrophysical Journal, 902, 20. https://doi.org/10.3847/1538-4357/abb2a4
[68] Moncuquet, M., et al. 2020, First In Situ Measurements of Electron Density and Temperature from Quasi-thermal Noise Spectroscopy with Parker Solar Probe/FIELDS, The Astrophysical Journal Supplement Series, 246, 44. https://doi.org/10.3847/1538-4365/ab5a84
[69] Morosan, D. E., & Gallagher, P. T. 2017. in Planetary Radio Emissions VIII, Characteristics of type III radio bursts and solar S bursts, eds. G. Fischer, G. Mann, M. Panchenko, & P. Zarka, 357
[70] Morosan, D. E., Kilpua, E. K. J., Carley, E. P., & Monstein, C. 2019, Variable emission mechanism of a Type IV radio burst, Astronomy and Astrophysics, 623, A63. https://doi.org/10.1051/0004-6361/201834510
[71] Morosan, D. E., et al. 2022, Exploring the Circular Polarisation of Low–Frequency Solar Radio Bursts with LOFAR, Solar Physics, 297. https://doi.org/10.1007/s11207-022-01976-9
[72] Musset, S., et al. 2021, Simulations of radio-wave anisotropic scattering to interpret type III radio burst data from Solar Orbiter, Parker Solar Probe, STEREO, and Wind, Astronomy and Astrophysics, 656, A34. https://doi.org/10.1051/0004-6361/202140998
[73] Ogawara, Y., et al. 1991, The SOLAR-A Mission - An Overview, Solar Physics, 136, 1. https://doi.org/10.1007/bf00151692
[74] Pesnell, W. D., Thompson, B. J., & Chamberlin, P. C. 2012, The Solar Dynamics Observatory (SDO), Solar Physics, 275, 3. https://doi.org/10.1007/s11207-011-9841-3
[75] Pick, M. 2005, in Solar and Space Weather Radiophysics: Current Status and Future Developments, eds. D. E. Gary, & C. U. Keller (Dordrecht: Springer Netherlands), 17
[76] Pulupa, M., et al. 2020, Statistics and Polarization of Type III Radio Bursts Observed in the Inner Heliosphere, The Astrophysical Journal Supplement Series, 246. https://doi.org/10.3847/1538-4365/ab5dc0
[77] Pulupa, M., et al. 2017, The Solar Probe Plus Radio Frequency Spectrometer: Measurement requirements, analog design, and digital signal processing, Journal of Geophysical Research (Space Physics), 122, 2836. https://doi.org/10.1002/2016ja023345
[78] Rahman, M. M., Cairns, I. H., & McCauley, P. I. 2020, Spectropolarimetric Imaging of Metric Type III Solar Radio Bursts, Solar Physics, 295, 51. https://doi.org/10.1007/s11207-020-01616-0
[79] Raouafi, N. E., et al. 2023, Parker Solar Probe: Four Years of Discoveries at Solar Cycle Minimum, Space Science Reviews, 219, 8. https://doi.org/10.1007/s11214-023-00952-4
[80] Reames, D. V., von Rosenvinge, T. T., & Lin, R. P. 1985, Solar He-3-rich events and nonrelativistic electron events - A new association, The Astrophysical Journal, 292, 716. https://doi.org/10.1086/163203
[81] Reber, G. 1944, Cosmic Static, The Astrophysical Journal, 100, 279. https://doi.org/10.1086/144668
[82] Reid, H. A. S., & Kontar, E. P. 2015, Stopping frequency of type III solar radio bursts in expanding magnetic flux tubes, Astronomy and Astrophysics, 577, A124. https://doi.org/10.1051/0004-6361/201425309
[83] Reid, H. A. S., & Kontar, E. P. 2017, Imaging spectroscopy of type U and J solar radio bursts with LOFAR, Astronomy & Astrophysics, 606, A141. https://doi.org/10.1051/0004-6361/201730701
[84] Reid, H. A. S., & Kontar, E. P. 2018, Solar type III radio burst time characteristics at LOFAR frequencies and the implications for electron beam transport, Astronomy and Astrophysics, 614, A69. https://doi.org/10.1051/0004-6361/201732298
[85] Reid, H. A. S., & Ratcliffe, H. 2014, A review of solar type III radio bursts, Research in Astronomy and Astrophysics, 14, 773. https://doi.org/10.1088/1674-4527/14/7/003
[86] Reiner, M. J., Fainberg, J., Kaiser, M. L., & Bougeret, J. L. 2007, Circular Polarization Observed in Interplanetary Type III Radio Storms, Solar Physics, 241, 351. https://doi.org/10.1007/s11207-007-0277-8
[87] Reiner, M. J., & Kaiser, M. L. 1999, High-frequency type II radio emissions associated with shocks driven by coronal mass ejections, Journal of Geophysical Research, 104, 16979. https://doi.org/10.1029/1999ja900143
[88] Robinson, P. A., & Cairns, I. H. 1998, Fundamental and Harmonic Emission in Type III Solar Radio Bursts - I. Emission at a Single Location or Frequency, Solar Physics, 181, 363. https://doi.org/10.1023/a:1005018918391
[89] Robinson, P. A., Cairns, I. H., & Gurnett, D. A. 1993, Clumpy Langmuir Waves in Type III Radio Sources: Comparison of Stochastic-Growth Theory with Observations, The Astrophysical Journal, 407, 790. https://doi.org/10.1086/172560
[90] Schou, J., et al. 2012, Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO), Solar Physics, 275, 229. https://doi.org/10.1007/s11207-011-9842-2
[91] Singh, Y. P., & Badruddin. 2006, Statistical considerations in superposed epoch analysis and its applications in space research, Journal of Atmospheric and Solar-Terrestrial Physics, 68, 803. https://doi.org/10.1016/j.jastp.2006.01.007
[92] Stanislavsky, A. A., Bubnov, I. N., Koval, A. A., & Yerin, S. N. 2021, Parker Solar Probe detects solar radio bursts related with a behind–the–limb active region, Astronomy & Astrophysics, 657. https://doi.org/10.1051/0004-6361/202141984
[93] Stewart, R. T., & Labrum, N. R. 1972, Meter-wavelength observations of the solar radio burst storm of August 17 22, 1968, Solar Physics, 27, 192. https://doi.org/10.1007/bf00151783
[94] Thejappa, G., & MacDowall, R. J. 2021, Observational Evidence for Beat Phenomenon in Complex Solar Type III Radio Bursts, The Astrophysical Journal, 912, 61. https://doi.org/10.3847/1538-4357/abee74
[95] Thompson, W. T. 2006, Coordinate systems for solar image data, Astronomy and Astrophysics, 449, 791. https://doi.org/10.1051/0004-6361:20054262
[96] Thompson, W. T., et al. 2003. in Innovative Telescopes and Instrumentation for Solar Astrophysics, COR1 inner coronagraph for STEREO-SECCHI, eds. S. L. Keil, & S. V. Avakyan, 1
[97] Treumann, R. A. 2006, The electron–cyclotron maser for astrophysical application, The Astronomy and Astrophysics Review, 13, 229. https://doi.org/10.1007/s00159-006-0001-y
[98] van Haarlem, M. P., et al. 2013, LOFAR: The LOw-Frequency ARray, Astronomy and Astrophysics, 556, A2. https://doi.org/10.1051/0004-6361/201220873
[99] Vecchio, A., et al. 2021, Solar Orbiter/RPW antenna calibration in the radio domain and its application to type III burst observations, Astronomy and Astrophysics, 656, A33. https://doi.org/10.1051/0004-6361/202140988
[100] Vidojevic, S., & Maksimovic, M. 2009, Preliminary Analysis of Type III Radio Bursts from Stereo/Waves Data, Publications de l′Observatoire Astronomique de Beograd, 86, 287.
[101] Vourlidas, A., et al. 2016, The Wide-Field Imager for Solar Probe Plus (WISPR), Space Science Reviews, 204, 83. https://doi.org/10.1007/s11214-014-0114-y
[102] Wang, M., Duan, C. C., Xie, R. X., & Yan, Y. H. 2003, Highly polarized Type III microwave bursts on 15 April 1998, Solar Physics, 212, 401. https://doi.org/10.1023/a:1022939203483
[103] Weiss, L. A. A., & Stewart, R. T. 1965, Solar radio bursts of spectral type V, Australian Journal of Physics, 18, 143. https://doi.org/10.1071/ph650143
[104] West, M. J., et al. 2023, Defining the Middle Corona, Solar Physics, 298, 78. https://doi.org/10.1007/s11207-023-02170-1
[105] White, S. 2007, Solar Radio Bursts and Space Weather, Asian J Phys, 16.
[106] White, S. M., & Kundu, M. R. 1997, Radio Observations of Gyroresonance Emission from Coronal Magnetic Fields, Solar Physics, 174, 31. https://doi.org/10.1023/A:1004975528106
[107] Wild, J. P., & McCready, L. L. 1950, Observations of the Spectrum of High-Intensity Solar Radiation at Metre Wavelengths. I. The Apparatus and Spectral Types of Solar Burst Observed, Australian Journal of Scientific Research A Physical Sciences, 3, 387. https://doi.org/10.1071/ch9500387
[108] Woods, T. N., et al. 2012, Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments, Solar Physics, 275, 115. https://doi.org/10.1007/s11207-009-9487-6
[109] Zhang, J., Reid, H. A. S., Krupar, V., Zucca, P., Dabrowski, B., & Krankowski, A. 2023, Deriving Large Coronal Magnetic Loop Parameters Using LOFAR J Burst Observations, Solar Physics, 298, 7. https://doi.org/10.1007/s11207-022-02096-0
[110] Zhang, P. J., Wang, C. B., & Ye, L. 2018, A type III radio burst automatic analysis system and statistic results for a half solar cycle with Nançay Decameter Array data, Astronomy & Astrophysics, 618, A165. https://doi.org/10.1051/0004-6361/201833260
[111] Zheleznyakov, V. V., & Zaitsev, V. V. 1968, The Origin of Type-V Solar Radio Bursts, Soviet Astronomy, 12, 14.
[112] Zlobec, P., & Thejappa, G. 1987, Type II Burst High Time Resolution and Polarization Characteristics at Frequencies Higher than 200 MHz, Hvar Observatory Bulletin, 11, 111. |