Zobrazeno 1 - 10
of 933
pro vyhledávání: '"Jess, D. A."'
Autor:
Berretti, M., Stangalini, M., Verth, G., Jafarzadeh, S., Jess, D. B., Berrilli, F., Grant, S. D. T., Duckenfield, T., Fedun, V.
It is well known that the dominant frequency of oscillations in the solar photosphere is $\approx$3 mHz, which is the result of global resonant modes pertaining to the whole stellar structure. However, analyses of the horizontal motions of nearly 1 m
Externí odkaz:
http://arxiv.org/abs/2407.03950
Autor:
Bate, W., Jess, D. B., Grant, S. D. T., Hillier, A., Skirvin, S. J., van Doorsselaere, T., Jafarzadeh, S., Wiegelmann, T., Duckenfield, T., Beck, C., Moore, T., Stangalini, M., Keys, P. H., Christian, D. J.
The magnetic geometry of the solar atmosphere, combined with projection effects, makes it difficult to accurately map the propagation of ubiquitous waves in fibrillar structures. These waves are of interest due to their ability to carry energy into t
Externí odkaz:
http://arxiv.org/abs/2405.15584
Autor:
Jafarzadeh, S., Schiavo, L. A. C., Fedun, V., Solanki, S. K., Stangalini, M., Calchetti, D., Verth, G., Jess, D. B., Grant, S. D. T., Ballai, I., Gafeira, R., Keys, P. H., Fleck, B., Morton, R. J., Browning, P. K., Silva, S. A., Appourchaux, T., Gandorfer, A., Gizon, L., Hirzberger, J., Kahil, F., Suárez, D. Orozco, Schou, J., Strecker, H., Iniesta, J. C. del Toro, Valori, G., Volkmer, R., Woch, J.
Publikováno v:
A&A 688, A2 (2024)
Solar pores are intense concentrations of magnetic flux that emerge through the Sun's photosphere. When compared to sunspots, they are much smaller in diameter and hence can be impacted and buffeted by neighbouring granular activity to generate signi
Externí odkaz:
http://arxiv.org/abs/2404.18717
Autor:
Jess, D. B., Grant, S. D. T., Bate, W., Liu, J., Jafarzadeh, S., Keys, P. H., Vieira, L. E. A., Lago, A. Dal, Guarnieri, F. L., Christian, D. J., Gilliam, D., Banerjee, D.
The solar physics community is entering a golden era that is ripe with next-generation ground- and space-based facilities. With ever-increasing resolving power stemming from the newest observational telescopes, it becomes more challenging to obtain (
Externí odkaz:
http://arxiv.org/abs/2312.00122
Autor:
T., Moore, J., Smartt S., M., Nicholl, S., Srivastav, F., Stevance H., B., Jess D., T., Grant S. D., D., Fulton M., L., Rhodes, A., Sim S., R., Hirai, P., Podsiadlowski, P., Anderson J., C., Ashall, W., Bate, R., Fender, P., Gutierrez C., A., Howell D., E., Huber M., C., Inserra, G., Leloudas, G., Monard L. A., E., Muller-Bravo T., J., Shappee B., W., Smith K., G., Terreran, J., Tonry, A., Tucker M., R., Young D., A., Aamer, -W., Chen T., F., Ragosta, L., Galbany, M., Gromadzki, L., Harvey, P., Hoeflich, C., McCully, M., Newsome, P., Gonzalez E., C., Pellegrino, P., Ramsden, M., Perez-Torres, J., Ridley E., X., Sheng, J, Weston
We present multi-wavelength photometry and spectroscopy of SN 2022jli, an unprecedented Type Ic supernova discovered in the galaxy NGC 157 at a distance of $\approx$ 23 Mpc. The multi-band light curves reveal many remarkable characteristics. Peaking
Externí odkaz:
http://arxiv.org/abs/2309.12750
Autor:
Grant, S. D. T., Jess, D. B., Dillon, C. J., Mathioudakis, M., Watson, C. A., Jackman, J. A. G., Jackson, D. G., Wheatley, P. J., Goad, M. R., Casewell, S. L., Anderson, D. R., Burleigh, M. R., West, R. G., Vines, J. I.
Previous examinations of fully-convective M-dwarf stars have highlighted enhanced rates of nanoflare activity on these distant stellar sources. However, the specific role the convective boundary, which is believed to be present for spectral types ear
Externí odkaz:
http://arxiv.org/abs/2309.10035
Autor:
Campbell, Ryan J., Keys, P H., Mathioudakis, M., Woeger, F., Schad, T. A., Tritschler, A., de Wijn, A. G., Smitha, H. N., Beck, C. A., Christian, D J., Jess, D. B., Erdelyi, R.
We present the first quiet Sun spectropolarimetric observations obtained with the Visible SpectroPolarimeter (ViSP) at the $4-$m Daniel K. Inouye Solar Telescope (DKIST). We recorded observations in a wavelength range that includes the magnetically s
Externí odkaz:
http://arxiv.org/abs/2309.05836
Autor:
Salina H. Goff, Dylan T. Bergstedt, Marie L. Feser, LauraKay Moss, Ted R. Mikuls, Jess D. Edison, V. Michael Holers, Laura Martinez‐Prat, Mary Ann R. Aure, Michael Mahler, Kevin D. Deane
Publikováno v:
ACR Open Rheumatology, Vol 6, Iss 9, Pp 587-597 (2024)
Objective Rheumatoid arthritis (RA) has a “pre‐RA” period in which multiple autoantibodies, including antibodies to citrullinated (cit) proteins (ACPA), rheumatoid factor (RF), anti–peptidyl arginine deiminase (anti‐PAD), among others, have
Externí odkaz:
https://doaj.org/article/f06de7f98462462fa48bdd3b89115bf0
Autor:
Albidah, A. B., Fedun, V., Aldhafeeri, A. A., Ballai, I., Jess, D. B., Brevis, W., Higham, J., Stangalini, M., Silva, S. S. A., MacBride, C. D., Verth, G.
Through their lifetime sunspots undergo a change in their area and shape and, as they decay, they fragment into smaller structures. Here, for the first time we analyze the spatial structure of magnetohydrodynamic (MHD) slow body and fast surface mode
Externí odkaz:
http://arxiv.org/abs/2305.19418
Autor:
Abdallah Abushehab, MD, Jess D. Rames, MD, Sara M. Hussein, MD, Alexandre Meira Pazelli, MD, Tori A. Sears, MS, Adam J. Wentworth, MS, MD, Jonathan M. Morris, MD, Basel A. Sharaf, MD, DDS
Publikováno v:
Plastic and Reconstructive Surgery, Global Open, Vol 12, Iss 10, p e6215 (2024)
Background:. Facial shape is significantly influenced by the underlying facial bony skeleton. Sexual dimorphisms in these structures are crucial for craniofacial, aesthetic, and gender-affirming surgery. Previous studies have examined the orbits and
Externí odkaz:
https://doaj.org/article/90828a857aeb4dbd8491b12e2a7616de