Study on solar sources and polar cap absorption events recorded in Antarctica
Particularly intense events occurred on the Sun in a period around minimum of solar activity during cycle 23. We investigated the characteristics of September 2005 and December 2006 events and the properties of the correlated observations of ionospheric absorption, obtained by a 30 MHz riometer inst...
| Main Authors: | , , , , |
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| Other Authors: | , , , , , , |
| Format: | Manuscript |
| Language: | English |
| Published: |
2007
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| Online Access: | http://hdl.handle.net/2122/3026 |
| _version_ | 1821725486345093120 |
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| author | Perrone, L. Parisi, M. Meloni, A. Damasso, M. Galliani, M. |
| author2 | Perrone, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Parisi, M.; Dipartimento di Fisica, Università degli Studi di Roma Tre Meloni, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Damasso, M.; Dipartimento di Fisica, Università degli Studi di Roma Tre Galliani, M.; Dipartimento di Fisica, Università degli Studi di Roma Tre Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Dipartimento di Fisica, Università degli Studi di Roma Tre |
| author_facet | Perrone, L. Parisi, M. Meloni, A. Damasso, M. Galliani, M. |
| author_sort | Perrone, L. |
| collection | Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) |
| description | Particularly intense events occurred on the Sun in a period around minimum of solar activity during cycle 23. We investigated the characteristics of September 2005 and December 2006 events and the properties of the correlated observations of ionospheric absorption, obtained by a 30 MHz riometer installed at Mario Zucchelli Station (MZS-Antarctica), and of geomagnetic activity recorded at Scott Base (Antarctica). Solar events are studied using the characteristics of CMEs measured with SoHO/LASCO coronagraphs and the temporal evolution of solar energetic protons in different energy ranges measured by GOES 11 spacecraft. Analysing these data, we have determined possible clues that could allow a forecast evaluation of the effects produced at the Earth’s orbit by the interplanetary perturbations. Moreover we have determined as these effects are finally observed on the Earth’s surface not only in the ionospheric absorption of radio waves and in the intense geomagnetic activity, but also as significant variations of cosmic ray modulation, even at high energies. Submitted 1.7. Osservazioni di alta e media atmosfera N/A or not JCR reserved |
| format | Manuscript |
| genre | Antarc* Antarctica |
| genre_facet | Antarc* Antarctica |
| geographic | Alta Scott Base Mario Zucchelli Mario Zucchelli Station |
| geographic_facet | Alta Scott Base Mario Zucchelli Mario Zucchelli Station |
| id | ftingv:oai:www.earth-prints.org:2122/3026 |
| institution | Open Polar |
| language | English |
| long_lat | ENVELOPE(166.766,166.766,-77.849,-77.849) ENVELOPE(164.123,164.123,-74.695,-74.695) ENVELOPE(164.117,164.117,-74.700,-74.700) |
| op_collection_id | ftingv |
| op_relation | Advances in Space Research Akasofu, S.J., Energy coupling between the solar wind and the magnetosphere, Space Sci. Rev, 28, 121, 1981. Arnoldy, R. L., Signature in the interplanetary for substorms, J. Geophys. Res., 76, 5189, 1971. Burlaga, L. F., Plunkett, S. P. & St Cyr, O.C., Successive CMEs and complex ejecta, J. Geophys. Res., 107, 1266, 2002. Cane, H. V., Richardson, I. G. &St Cyr O.C., Coronal mass ejections, interplanetary ejecta and geomagnetic storms, Geophys. Res. Lett., 27, 3591,2000. Cane H. V., R. A. Mewaldt, C. M. S. Cohen, T. T. von Rosenvinge, Role of flares and shocks in determining solar energetic particle abundances, J. Geophys. Res., 111, A06S90, 2006. Collis, P.N. and Rietveld, M.N.: Mesospheric observations with the EISCAT UHF radar during polar cap absorption events: electron densities and negative ions, Ann. Geophysicae, 8, 809-824, 1990. Gopalswamy N., S. Yashiro, S. Krucker, G. Stenborg, R. A. Howard , Intensity variation of large solar energetic particle events associated with coronal mass ejections, J. Geophys. Res., 109, A12105,2004. Gopalswamy, N, Yashiro, S. & Akiyama, S., Geoeffectiveness of halo coronal mass ejections, J. Geophys. Res.,112, 6, 2007. Hargreaves, J.K., Shirochkov, A.V. and Farmer, A.D.: The polar cap absorption event of 19-21 March 1990: recombination coefficients, the twilight transition and midday recovery, J. Atmos. Terr. Phys., 55, 857-862, 1993. Hudson, H.S., Lemen, J. R. , Sr. Cyr, O.C., Sterling, A.C. & Webb, D. F., Hudson, J. G., Y. Xie, Cloud condensation nuclei measurements in the high troposphere and in jet aircraft exhaust. Geophys. Res. Lett., 25, 2481, 1998. Monn, Y. J., Cho, K. S, Dryer M., Kim, Y. H.,Bong, S.C., Chae, J. & Park, Y. D., New geoeffectiveness parameters for very fast coronal mass ejections, Astrophys. J., 624,404, 2005. Perrone L., L. Alfonsi, V. Romano and G. De Franceschi: “ Polar cap absorption events of November 2001 at Terra Nova Bay, Antartica”, Annales Geophysicae, 22, 1633-1648, 2004. Ranta, H., Ranta, A., Yousef, S.M., Burns, J. and Stauning, P.: D-region observations of polar cap absorption events during the EISCAT operation in 1981-1989, J. Atmos. Terr. Phys, 55, 751-766, 1993. Reid, G.H.: Polar Cap Absorption – Observations and Theory, Fundamentals of Cosmic Physics, 1, 167–204, 1974. St. Cyr, O.C. et al. , Properties of coronal mass ejections SOHO LASCO observations from January 1996 to January 1998, J. Gephys. Res. 105, 18169, 2000 Sellers, B., Hanser, F.A., Stroscio, M.A. and Yates, G.K.: The night and day relationships between polar cap riometer absorption and solar protons, Radio Sci., 5, 779-789, 1977. http://hdl.handle.net/2122/3026 |
| op_rights | restricted |
| publishDate | 2007 |
| record_format | openpolar |
| spelling | ftingv:oai:www.earth-prints.org:2122/3026 2025-01-16T19:17:30+00:00 Study on solar sources and polar cap absorption events recorded in Antarctica Perrone, L. Parisi, M. Meloni, A. Damasso, M. Galliani, M. Perrone, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Parisi, M.; Dipartimento di Fisica, Università degli Studi di Roma Tre Meloni, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Damasso, M.; Dipartimento di Fisica, Università degli Studi di Roma Tre Galliani, M.; Dipartimento di Fisica, Università degli Studi di Roma Tre Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Dipartimento di Fisica, Università degli Studi di Roma Tre 2007 http://hdl.handle.net/2122/3026 en eng Advances in Space Research Akasofu, S.J., Energy coupling between the solar wind and the magnetosphere, Space Sci. Rev, 28, 121, 1981. Arnoldy, R. L., Signature in the interplanetary for substorms, J. Geophys. Res., 76, 5189, 1971. Burlaga, L. F., Plunkett, S. P. & St Cyr, O.C., Successive CMEs and complex ejecta, J. Geophys. Res., 107, 1266, 2002. Cane, H. V., Richardson, I. G. &St Cyr O.C., Coronal mass ejections, interplanetary ejecta and geomagnetic storms, Geophys. Res. Lett., 27, 3591,2000. Cane H. V., R. A. Mewaldt, C. M. S. Cohen, T. T. von Rosenvinge, Role of flares and shocks in determining solar energetic particle abundances, J. Geophys. Res., 111, A06S90, 2006. Collis, P.N. and Rietveld, M.N.: Mesospheric observations with the EISCAT UHF radar during polar cap absorption events: electron densities and negative ions, Ann. Geophysicae, 8, 809-824, 1990. Gopalswamy N., S. Yashiro, S. Krucker, G. Stenborg, R. A. Howard , Intensity variation of large solar energetic particle events associated with coronal mass ejections, J. Geophys. Res., 109, A12105,2004. Gopalswamy, N, Yashiro, S. & Akiyama, S., Geoeffectiveness of halo coronal mass ejections, J. Geophys. Res.,112, 6, 2007. Hargreaves, J.K., Shirochkov, A.V. and Farmer, A.D.: The polar cap absorption event of 19-21 March 1990: recombination coefficients, the twilight transition and midday recovery, J. Atmos. Terr. Phys., 55, 857-862, 1993. Hudson, H.S., Lemen, J. R. , Sr. Cyr, O.C., Sterling, A.C. & Webb, D. F., Hudson, J. G., Y. Xie, Cloud condensation nuclei measurements in the high troposphere and in jet aircraft exhaust. Geophys. Res. Lett., 25, 2481, 1998. Monn, Y. J., Cho, K. S, Dryer M., Kim, Y. H.,Bong, S.C., Chae, J. & Park, Y. D., New geoeffectiveness parameters for very fast coronal mass ejections, Astrophys. J., 624,404, 2005. Perrone L., L. Alfonsi, V. Romano and G. De Franceschi: “ Polar cap absorption events of November 2001 at Terra Nova Bay, Antartica”, Annales Geophysicae, 22, 1633-1648, 2004. Ranta, H., Ranta, A., Yousef, S.M., Burns, J. and Stauning, P.: D-region observations of polar cap absorption events during the EISCAT operation in 1981-1989, J. Atmos. Terr. Phys, 55, 751-766, 1993. Reid, G.H.: Polar Cap Absorption – Observations and Theory, Fundamentals of Cosmic Physics, 1, 167–204, 1974. St. Cyr, O.C. et al. , Properties of coronal mass ejections SOHO LASCO observations from January 1996 to January 1998, J. Gephys. Res. 105, 18169, 2000 Sellers, B., Hanser, F.A., Stroscio, M.A. and Yates, G.K.: The night and day relationships between polar cap riometer absorption and solar protons, Radio Sci., 5, 779-789, 1977. http://hdl.handle.net/2122/3026 restricted interplanetary perturbations 05. General::05.07. Space and Planetary sciences::05.07.01. Solar-terrestrial interaction manuscript 2007 ftingv 2022-07-29T06:04:38Z Particularly intense events occurred on the Sun in a period around minimum of solar activity during cycle 23. We investigated the characteristics of September 2005 and December 2006 events and the properties of the correlated observations of ionospheric absorption, obtained by a 30 MHz riometer installed at Mario Zucchelli Station (MZS-Antarctica), and of geomagnetic activity recorded at Scott Base (Antarctica). Solar events are studied using the characteristics of CMEs measured with SoHO/LASCO coronagraphs and the temporal evolution of solar energetic protons in different energy ranges measured by GOES 11 spacecraft. Analysing these data, we have determined possible clues that could allow a forecast evaluation of the effects produced at the Earth’s orbit by the interplanetary perturbations. Moreover we have determined as these effects are finally observed on the Earth’s surface not only in the ionospheric absorption of radio waves and in the intense geomagnetic activity, but also as significant variations of cosmic ray modulation, even at high energies. Submitted 1.7. Osservazioni di alta e media atmosfera N/A or not JCR reserved Manuscript Antarc* Antarctica Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) Alta Scott Base ENVELOPE(166.766,166.766,-77.849,-77.849) Mario Zucchelli ENVELOPE(164.123,164.123,-74.695,-74.695) Mario Zucchelli Station ENVELOPE(164.117,164.117,-74.700,-74.700) |
| spellingShingle | interplanetary perturbations 05. General::05.07. Space and Planetary sciences::05.07.01. Solar-terrestrial interaction Perrone, L. Parisi, M. Meloni, A. Damasso, M. Galliani, M. Study on solar sources and polar cap absorption events recorded in Antarctica |
| title | Study on solar sources and polar cap absorption events recorded in Antarctica |
| title_full | Study on solar sources and polar cap absorption events recorded in Antarctica |
| title_fullStr | Study on solar sources and polar cap absorption events recorded in Antarctica |
| title_full_unstemmed | Study on solar sources and polar cap absorption events recorded in Antarctica |
| title_short | Study on solar sources and polar cap absorption events recorded in Antarctica |
| title_sort | study on solar sources and polar cap absorption events recorded in antarctica |
| topic | interplanetary perturbations 05. General::05.07. Space and Planetary sciences::05.07.01. Solar-terrestrial interaction |
| topic_facet | interplanetary perturbations 05. General::05.07. Space and Planetary sciences::05.07.01. Solar-terrestrial interaction |
| url | http://hdl.handle.net/2122/3026 |