Search Results - "FRY, D. C"

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  1. 1

    On the Evolution of Coronal Mass Ejections in the Interplanetary Medium by Howard, T. A, Fry, C. D, Johnston, J. C, Webb, D. F

    Published in The Astrophysical journal (20-09-2007)
    “…Two coronal mass ejections (CMEs) are presented which were tracked through the LASCO field of view (FOV) within 30 R [unk] and later as interplanetary CMEs…”
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  2. 2

    Three-dimensional global simulation of interplanetary coronal mass ejection propagation from the Sun to the heliosphere: Solar event of 12 May 1997 by Wu, Chin-Chun, Fry, C. D., Wu, S. T., Dryer, M., Liou, Kan

    “…A newly developed hybrid code, HAFv.2+3DMHD, that combines two simulation codes, Hakamada‐Akasofu‐Fry code version 2 (HAFv.2) and a fully three‐dimensional…”
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  3. 3

    Forecasting solar wind structures and shock arrival times using an ensemble of models by Fry, C. D., Dryer, M., Smith, Z., Sun, W., Deehr, C. S., Akasofu, S.-I.

    “…Forecasting the time of arrival at Earth of interplanetary shocks following solar metric type II activity is an important first step in the establishment of an…”
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  4. 4

    Operational validation of HAFv2's predictions of interplanetary shock arrivals at Earth: Declining phase of Solar Cycle 23 by Smith, Z. K., Dryer, M., McKenna‐Lawlor, S. M. P., Fry, C. D., Deehr, C. S., Sun, W.

    “…This is the third in a series of papers showing the performance of the Hakamada‐Akasofu‐Fry version 2 (HAFv2) model in predicting, in the operational…”
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  5. 5

    Improvements to the HAF solar wind model for space weather predictions by Fry, C. D., Sun, W., Deehr, C. S., Dryer, M., Smith, Z., Akasofu, S.‐I., Tokumaru, M., Kojima, M.

    “…We have assembled and tested, in real time, a space weather modeling system that starts at the Sun and extends to the Earth through a set of coupled, modular…”
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  6. 6

    Near real-time predictions of the arrival at Earth of flare-related shocks during Solar Cycle 23 by McKenna-Lawlor, S. M. P., Dryer, M., Kartalev, M. D., Smith, Z., Fry, C. D., Sun, W., Deehr, C. S., Kecskemety, K., Kudela, K.

    “…The arrival times at Earth of 166 flare‐related shocks identified exiting the Sun (using metric radio drift data) during the maximum phase of Solar Cycle 23,…”
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  7. 7

    Statistical analysis of corotating interaction regions and their geoeffectiveness during solar cycle 23 by Zhang, Y., Sun, W., Feng, X. S., Deehr, C. S., Fry, C. D., Dryer, M.

    “…This is an investigation of the effects of corotating interaction regions (CIRs) in the heliosphere (<1 AU) on geomagnetic disturbances during solar cycle 23…”
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  8. 8

    Effects of solar X-ray flares in the E region ionosphere of Mars: First model results by Haider, S. A., McKenna-Lawlor, S. M. P., Fry, C. D., Jain, Rajmal, Joshipura, K. N.

    “…We have used radio occultation data obtained from Mars Global Surveyor (MGS) at high latitudes (65.3°–65.6°N, 69.3°–69.6°N and 76.4°–77.5°N) to study the…”
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  9. 9

    Study of CME Propagation in the Inner Heliosphere: SOHO LASCO, SMEI and STEREO HI Observations of the January 2007 Events by Webb, D. F., Howard, T. A., Fry, C. D., Kuchar, T. A., Odstrcil, D., Jackson, B. V., Bisi, M. M., Harrison, R. A., Morrill, J. S., Howard, R. A., Johnston, J. C.

    Published in Solar physics (01-05-2009)
    “…We are investigating the geometric and kinematic characteristics of interplanetary coronal mass ejections (ICMEs) using data obtained by the LASCO…”
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  10. 10

    A practical database method for predicting arrivals of “average” interplanetary shocks at Earth by Feng, X. S., Zhang, Y., Sun, W., Dryer, M., Fry, C. D., Deehr, C. S.

    “…A practical database method for predicting the interplanetary shock arrival time at L1 point is presented here. First, a shock transit time database…”
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  11. 11
  12. 12

    Chandra Observations of Comet 2P/Encke 2003: First Detection of a Collisionally Thin, Fast Solar Wind Charge Exchange System by Lisse, C. M, Christian, D. J, Dennerl, K, Wolk, S. J, Bodewits, D, Hoekstra, R, Combi, M. R, Mäkinen, T, Dryer, M, Fry, C. D, Weaver, H

    Published in The Astrophysical journal (20-12-2005)
    “…We report the results of 15 hr of Chandra observations of comet 2P/Encke 2003 on November 24. X-ray emission from comet Encke was resolved on scales of…”
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  13. 13

    Annual TEC variation in the equatorial anomaly region during the solar minimum: September 1996–August 1997 by Wu, Chin-Chun, Fry, C.D., Liu, J.-Y., Liou, K., Tseng, C.-L.

    “…The ionospheric total electron content (TEC) in the equatorial anomaly region is studied by analyzing dual-frequency signals from the global position system…”
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  14. 14

    A statistical study of the performance of the Hakamada-Akasofu-Fry version 2 numerical model in predicting solar shock arrival times at Earth during different phases of solar cycle 23 by MCKENNA-LAWLOR, S. M. P, FRY, C. D, DRYER, M, HEYNDERICKX, D, KECSKEMETY, K, KUDELA, K, BALAZ, J

    Published in Annales geophysicae (1988) (27-02-2012)
    “…The performance of the Hakamada Akasofu-Fry, version 2 (HAFv.2) numerical model, which provides predictions of solar shock arrival times at Earth, was…”
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  15. 15

    Examination of type II origin with SOHO/LASCO observations by Cho, K.-S., Moon, Y.-J., Dryer, M., Shanmugaraju, A., Fry, C. D., Kim, Y.-H., Bong, S.-C., Park, Y.-D.

    “…We examine a possibility that metric type II solar radio bursts are all caused by coronal mass ejection (CME) generated shocks. For this we consider 129 type…”
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  16. 16

    Effects of the interaction and evolution of interplanetary shocks on “background” solar wind speeds by Wu, Chin-Chun, Feng, X. S., Wu, S. T., Dryer, M., Fry, C. D.

    “…Solar wind speed plays an important role in the study of space weather prediction. Some workers have used it for measuring the arrival time of solar…”
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  17. 17
  18. 18

    A statistical comparison of interplanetary shock and CME propagation models by Cho, K.-S., Moon, Y.-J., Dryer, M., Fry, C. D., Park, Y.-D., Kim, K.-S.

    “…We have compared the prediction capability of two types of Sun‐Earth connection models: (1) ensemble of physics‐based shock propagation models (STOA, STOA‐2,…”
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  19. 19

    Heliospheric energetic particle observations during the October–November 2003 events by Lario, D., Decker, R. B., Livi, S., Krimigis, S. M., Roelof, E. C., Russell, C. T., Fry, C. D.

    “…The intense level of solar activity recorded from 19 October to 12 November 2003 led to unusually high energetic particle intensities observed throughout the…”
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  20. 20

    Flare-generated shock evolution and geomagnetic storms during the “Halloween 2003 epoch”: 29 October to 2 November by Wu, Chin-Chun, Wu, S. T., Dryer, M., Fry, C. D., Berdichevsky, D., Smith, Z., Detman, T., Gopalswamy, N., Skoug, R., Zurbuchen, T., Smith, C.

    “…The October/November 2003 (“Halloween 2003”) epoch of intense solar flares provided an opportunity to test the results of earlier parametric 1.5 MHD studies of…”
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