Zobrazeno 1 - 10
of 110
pro vyhledávání: '"Towner, M. C."'
Autor:
Sansom, E. K., Devillepoix, H. A. R., Yamamoto, M. -Y., Abe, S., Nozawa, S., Towner, M. C., Cupák, M., Hiramatsu, Y., Kawamura, T., Fujita, K., Yoshikawa, M., Ishihara, Y., Hamama, I., Segawa, N., Kakinami, Y., Furumoto, M., Katao, H., Inoue, Y., Cool, A., Bonning, G., Howie, R. M., Bland, P. A.
On 5th December 2020 at 17:28 UTC, the Japan Aerospace Exploration Agency's Hayabusa-2 sample return capsule came back to the Earth. It re-entered the atmosphere over South Australia, visible for 53 seconds as a fireball from near the Northern Territ
Externí odkaz:
http://arxiv.org/abs/2111.02235
Autor:
Towner, M. C., Jansen-Sturgeon, T., Cupak, M., Sansom, E. K., Devillepoix, H. A. R., Bland, P. A., Howie, R. M, Paxman, J. P., Benedix, G. K., Hartig, B. A. D.
Fireball networks are used to recover meteorites, with the context of orbits. Observations from these networks cover the bright flight, where the meteoroid is luminescent, but to recover a fallen meteorite, these observations must often be predicted
Externí odkaz:
http://arxiv.org/abs/2108.04397
Autor:
Shober, P. M., Jansen-Sturgeon, T., Bland, P. A., Devillepoix, H. A. R., Sansom, E. K., Towner, M. C., Cupák, M., Howie, R. M., Hartig, B. A. D.
Based on telescopic observations of Jupiter-family comets (JFCs), there is predicted to be a paucity of objects at sub-kilometre sizes. However, several bright fireballs and some meteorites have been tenuously linked to the JFC population, showing me
Externí odkaz:
http://arxiv.org/abs/2008.08848
Autor:
Sansom, E. K., Bland, P. A., Towner, M. C., Devillepoix, H. A. R. D., Cupak, M., Howie, R. M., Jansen-Sturgeon, T., Cox, M. A., Hartig, B. A. D., Paxman, J. P., Benedix, G., Forman, L. V.
On the 27th of November 2015, at 10:43:45.526 UTC, a fireball was observed across South Australia by ten Desert Fireball Network observatories lasting 6.1 s. A $\sim37$ kg meteoroid entered the atmosphere with a speed of 13.68$\pm0.09\,\mbox{km s}^{-
Externí odkaz:
http://arxiv.org/abs/2006.07151
Autor:
Devillepoix, H. A. R., Cupák, M., Bland, P. A., Sansom, E. K., Towner, M. C., Howie, R. M., Hartig, B. A. D., Jansen-Sturgeon, T., Shober, P. M., Anderson, S. L., Benedix, G. K., Busan, D., Sayers, R., Jenniskens, P., Albers, J., Herd, C. D. K., Hill, P. J. A., Brown, P. G., Krzeminski, Z., Osinski, G. R., Aoudjehane, H. Chennaoui, Benkhaldoun, Z., Jabiri, A., Guennoun, M., Barka, A., Darhmaoui, H., Daly, L., Collins, G. S., McMullan, S., Suttle, M. D., Ireland, T., Bonning, G., Baeza, L., Alrefay, T. Y., Horner, J., Swindle, T. D., Hergenrother, C. W., Fries, M. D., Tomkins, A., Langendam, A., Rushmer, T., O'Neill, C., Janches, D., Hormaechea, J. L., Shaw, C., Young, J. S., Alexander, M., Mardon, A. D., Tate, J. R.
The world's meteorite collections contain a very rich picture of what the early Solar System would have been made of, however the lack of spatial context with respect to their parent population for these samples is an issue. The asteroid population i
Externí odkaz:
http://arxiv.org/abs/2004.01069
Autor:
Shober, P. M., Jansen-Sturgeon, T., Sansom, E. K., Devillepoix, H. A. R., Bland, P. A., Cupák, M., Towner, M. C., Howie, R. M., Hartig, B. A. D.
Objects gravitationally captured by the Earth-Moon system are commonly called temporarily captured orbiters (TCOs), natural Earth satellites, or minimoons. TCOs are a crucially important subpopulation of near-Earth objects (NEOs) to understand becaus
Externí odkaz:
http://arxiv.org/abs/1912.01894
Autor:
Shober, P. M., Jansen-Sturgeon, T., Sansom, E. K., Devillepoix, H. A. R., Towner, M. C., Bland, P. A., Cupák, M., Howie, R. M., Hartig, B. A. D.
For centuries extremely-long grazing fireball displays have fascinated observers and inspired people to ponder about their origins. The Desert Fireball Network (DFN) is the largest single fireball network in the world, covering about one third of Aus
Externí odkaz:
http://arxiv.org/abs/1912.01895
Autor:
Andreoni, I., Ackley, K., Cooke, J., Acharyya, A., Allison, J. R., Anderson, G. E., Ashley, M. C. B., Baade, D., Bailes, M., Bannister, K., Beardsley, A., Bessell, M. S., Bian, F., Bland, P. A., Boer, M., Booler, T., Brandeker, A., Brown, I. S., Buckley, D., Chang, S. -W., Coward, D. M., Crawford, S., Crisp, H., Crosse, B., Cucchiara, A., Cupák, M., de Gois, J. S., Deller, A., Devillepoix, H. A. R., Dobie, D., Elmer, E., Emrich, D., Farah, W., Farrell, T. J., Franzen, T., Gaensler, B. M., Galloway, D. K., Gendre, B., Giblin, T., Goobar, A., Green, J., Hancock, P. J., Hartig, B. A. D., Howell, E. J., Horsley, L., Hotan, A., Howie, R. M., Hu, L., Hu, Y., James, C. W., Johnston, S., Johnston-Hollitt, M., Kaplan, D. L., Kasliwal, M., Keane, E. F., Kenney, D., Klotz, A., Lau, R., Laugier, R., Lenc, E., Li, X., Liang, E., Lidman, C., Luvaul, L. C., Lynch, C., Ma, B., Macpherson, D., Mao, J., McClelland, D. E., McCully, C., Möller, A., Morales, M. F., Morris, D., Murphy, T., Noysena, K., Onken, C. A., Orange, N. B., Oslowski, S., Pallot, D., Paxman, J., Potter, S. B., Pritchard, T., Raja, W., Ridden-Harper, R., Romero-Colmenero, E., Sadler, E. M., Sansom, E. K., Scalzo, R. A., Schmidt, B. P., Scott, S. M., Seghouani, N., Shang, Z., Shannon, R. M., Shao, L., Shara, M. M., Sharp, R., Sokolowski, M., Sollerman, J., Staff, J., Steele, K., Sun, T., Suntzeff, N. B., Tao, C., Tingay, S., Towner, M. C., Thierry, P., Trott, C., Tucker, B. E., Väisänen, P., Krishnan, V. Venkatraman, Walker, M., Wang, L., Wang, X., Wayth, R., Whiting, M., Williams, A., Williams, T., Wolf, C., Wu, C., Wu, X., Yang, J., Yuan, X., Zhang, H., Zhou, J., Zovaro, H.
The discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era of multi-messenger astronomy. In this paper, we present follow-up obs
Externí odkaz:
http://arxiv.org/abs/1710.05846
Autor:
Schaffnit, S. B., Page, A. E., Lynch, R., Spake, L., Sear, R., Sosis, R., Shaver, J., Alam, N., Towner, M. C., Shenk, M. K.
Publikováno v:
Evolutionary Human Sciences; 2023, Vol. 5, p1-19, 19p
