Zobrazeno 1 - 10
of 603
pro vyhledávání: '"Holman G"'
Autor:
Lin, Y. -T., Burritt, T. H., Claessens, C., Holman, G., Kallander, M., Machado, E., Minter, L. I., Ostertag, R., Parno, D. S., Pedersen, J., Peterson, D. A., Robertson, R. G. H., Smith, E. B., Van Wechel, T. D., Hernández, A. P. Vizcaya
Publikováno v:
Phys. Rev. Lett. 124, 222502 (2020)
The beta decay of tritium in the form of molecular TT is the basis of sensitive experiments to measure neutrino mass. The final-state electronic, vibrational, and rotational excitations modify the beta spectrum significantly, and are obtained from th
Externí odkaz:
http://arxiv.org/abs/2001.11671
Autor:
Lin, R. P., Caspi, A., Krucker, S., Hudson, H., Hurford, G., Bandler, S., Christe, S., Davila, J., Dennis, B., Holman, G., Milligan, R., Shih, A. Y., Kahler, S., Kontar, E., Wiedenbeck, M., Cirtain, J., Doschek, G., Share, G. H., Vourlidas, A., Raymond, J., Smith, D. M., McConnell, M., Emslie, G.
Major solar eruptive events (SEEs), consisting of both a large flare and a near simultaneous large fast coronal mass ejection (CME), are the most powerful explosions and also the most powerful and energetic particle accelerators in the solar system,
Externí odkaz:
http://arxiv.org/abs/1311.5243
Context: Solar flare hard X-rays (HXRs) are thought to be produced by nonthermal coronal electrons stopping in the chromosphere, or remaining trapped in the corona. The collisional thick target model (CTTM) predicts that sources produced by harder po
Externí odkaz:
http://arxiv.org/abs/1305.1574
For a solar flare occurring on 2010 November 3, we present observations using several SDO/AIA extreme-ultraviolet (EUV) passbands of an erupting flux rope followed by inflows sweeping into a current sheet region. The inflows are soon followed by outf
Externí odkaz:
http://arxiv.org/abs/1111.1945
Autor:
Kontar, E. P., Brown, J. C., Emslie, A. G., Hajdas, W., Holman, G. D., Hurford, G. J., Kasparova, J., Mallik, P. C. V., Massone, A. M., McConnell, M. L., Piana, M., Prato, M., Schmahl, E. J., Suarez-Garcia, E.
X-radiation from energetic electrons is the prime diagnostic of flare-accelerated electrons. The observed X-ray flux (and polarization state) is fundamentally a convolution of the cross-section for the hard X-ray emission process(es) in question with
Externí odkaz:
http://arxiv.org/abs/1110.1755
Publikováno v:
Astrophys.J.659:750-757,2007
The energy released in a solar flare is partitioned between thermal and non-thermal particle energy and lost to thermal conduction and radiation over a broad range of wavelengths. It is difficult to determine the conductive losses and the energy radi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701359
Autor:
Holman, G. Paul
Publikováno v:
Connections, 2004 Sep 01. 3(3), 85-98.
Externí odkaz:
https://www.jstor.org/stable/26323053
Publikováno v:
In International Journal of Orthopaedic and Trauma Nursing 2010 14(1):18-29
Publikováno v:
In Journal of Orthopaedic Nursing 2009 13(4):172-182
Frozen fungi: cryogenic storage is an effective method to store Fusarium cultures for the long‐term.
Publikováno v:
Annals of Applied Biology. Sep2018, Vol. 173 Issue 2, p133-140. 9p.