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Cluster Hot Flow Anomaly Observations During Solar Cycle Minimum

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Book cover The Cluster Active Archive

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Abstract

Hot flow anomalies (HFAs) are studied using observations of the FGM magnetometer and the CIS plasma detector aboard the four Cluster spacecraft. Previously we studied several specific features of tangential discontinuities on the basis of Cluster measurements in February–April 2003 and discovered a new condition for forming HFAs that is the solar wind speed is higher than the average. However during the whole spring season of 2003, the solar wind speed was higher than average. In this study we analyse HFAs detected in 2007, the year of solar cycle minimum. Our earlier result was confirmed: the higher solar wind speed is a real condition for HFA formation; furthermore this constraint is independent of Schwartz et al.’s condition for HFA formation.

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References

  1. G. Erdős and A. Balogh. In situ observations of magnetic field fluctuations. Advances in Space Research, 35:625–635, 2005.

    Article  ADS  Google Scholar 

  2. G. Facskó, K. Kecskeméty, G. Erdős, M. Tátrallyay, P. W. Daly, and I. Dandouras. A statistical study of hot flow anomalies using Cluster data. Advances in Space Research, 41:1286–1291, 2008.

    Article  ADS  Google Scholar 

  3. K. Kecskeméty, G. Erdős, G. Facskó, M. Tátrallyay, I. Dandouras, P. Daly, and K. Kudela. Distributions of suprathermal ions near hot flow anomalies observed by RAPID aboard Cluster. Advances in Space Research, 38:1587–1594, 2006.

    Article  ADS  Google Scholar 

  4. Y. Lin. Global hybrid simulation of hot flow anomalies near the bow shock and in the magnetosheath. Planetary and Space Science, 50:577–591, 2002.

    Article  ADS  Google Scholar 

  5. E. A. Lucek, T. S. Horbury, A. Balogh, I. Dandouras, and H. Rème. Cluster observations of hot flow anomalies. Journal of Geophysical Research (Space Physics), 109(A6):207, 2004.

    Google Scholar 

  6. Z. Németh. Particle acceleration at the interaction of shocks and discontinuities. In Proceedings of 30th International Cosmic Ray Conference, 2007.

    Google Scholar 

  7. G. Paschmann and P. W. Daly, editors. Analysis Methods for Multi-Spacecraft Data, chapter Shock and Discontinuity Parameters, pages 249–270. ISSI/ESA, 1998.

    Google Scholar 

  8. S. J. Schwartz, C. P. Chaloner, D. S. Hall, P. J. Christiansen, and A. D. Johnstones. An active current sheet in the solar wind. Nature, 318:269–271, 1985.

    Article  ADS  Google Scholar 

  9. S. J. Schwartz, G. Paschmann, N. Sckopke, T. M. Bauer, M. Dunlop, A. N. Fazakerley, and M. F. Thomsen. Conditions for the formation of hot flow anomalies at Earth’s bow shock. Journal of Geophysical Research, 105:12639–12650, 2000.

    Article  ADS  Google Scholar 

  10. D.G. Sibeck, N.L. Borodkova, S.J. Schwartz, C.J. Owen, R. Kessel, S. Kokubun, R.P. Lepping, R. Lin, K. Liou, H. Lühr, R.W. McEntire, C.-I. Meng, T. Mukai, Z. Nemecek, G. Parks, T.D. Phan, S.A. Romanov, J. Safrankova, J.-A. Sauvaud, H.J. Singer, S.I. Solovyev, A. Szabo, K. Takahashi, D.J. Williams, K. Yumoto, and G.N. Zastenker. Comprehensive study of the magnetospheric response to a hot flow anomaly. Journal of Geophysical Research, 104:4577–4594, 1999.

    Article  ADS  Google Scholar 

  11. D. G. Sibeck, T.-D. Phan, R. Lin, R. P. Lepping, and A. Szabo. Wind observations of foreshock cavities: A case study. Journal of Geophysical Research (Space Physics), 107:4–1, 2002.

    Google Scholar 

  12. B. U. Ö. Sonnerup and M. Scheible. Minimum and maximum variance analysis. In G. Paschmann and S. J. Schwartz, editors, ISSI Book on Analysis Methods for Multi-Spacecraft Data, pages 185–220. ISSI, 1998.

    Google Scholar 

  13. J. Šafránková, L. Přech, Z. Němeček, D. G. Sibeck, and T. Mukai. Magnetosheath response to the interplanetary magnetic field tangential discontinuity. Journal of Geophysical Research, 105:25113–25122, 2000.

    Article  ADS  Google Scholar 

  14. M. F. Thomsen,, V. A. Thomas, D. Winske, J. T. Gosling, M. H. Farris, and C. T. Russell. Observational test of hot flow abnomaly formation by the interaction of s magnetic discontinuity with the bow shock. Journal of Geophysical Research, 98(A9):15319–15330, 1993.

    Article  ADS  Google Scholar 

  15. M. F. Thomsen, J. T. Gosling, S. A. Fuselier, S. J. Bame, and C. T. Russell. Hot, diamagnetic cavities upstream from the earth’s bow shock. Journal of Geophysical Research, 91:2961–2973, 1986.

    Article  ADS  Google Scholar 

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Acknowledgements

The authors thank the OTKA grant K75640 of the Hungarian Scientific Research Fund for support and the Cluster FGM, CIS and ACE MAG, SWEPAM teams for providing data for this study.

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Correspondence to G. Facskó .

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Facskó, G., Tátrallyay, M., Erdős, G., Dandouras, I. (2010). Cluster Hot Flow Anomaly Observations During Solar Cycle Minimum. In: Laakso, H., Taylor, M., Escoubet, C. (eds) The Cluster Active Archive. Astrophysics and Space Science Proceedings. Springer, Dordrecht. https://doi.org/10.1007/978-90-481-3499-1_25

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  • DOI: https://doi.org/10.1007/978-90-481-3499-1_25

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  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-3498-4

  • Online ISBN: 978-90-481-3499-1

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