Search Results - "Ciaravella, A"

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  1. 1

    Synthesis of Complex Organic Molecules in Soft X-Ray Irradiated Ices by Ciaravella, A., Jiménez-Escobar, A., Cecchi-Pestellini, C., Huang, C. H., Sie, N. E., Caro, G. M. Muñoz, Chen, Y. J.

    Published in The Astrophysical journal (01-07-2019)
    “…We study the chemical evolution of H2O:CO:NH3 ice mixtures irradiated with soft X-rays, in the range of 250-1250 eV. We identify many nitrogen-bearing…”
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    Journal Article
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    The Current Sheet Associated with the 2003 November 4 Coronal Mass Ejection: Density, Temperature, Thickness, and Line Width by Ciaravella, A, Raymond, J. C

    Published in The Astrophysical journal (20-10-2008)
    “…In the wake of the 2003 November 4 coronal mass ejection associated with the largest solar flare of the last sunspot cycle, a current sheet (CS) was observed…”
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    A stellar flare−coronal mass ejection event revealed by X-ray plasma motions by Argiroffi, C., Reale, F., Drake, J. J., Ciaravella, A., Testa, P., Bonito, R., Miceli, M., Orlando, S., Peres, G.

    Published in Nature astronomy (01-08-2019)
    “…Coronal mass ejections (CMEs), often associated with flares 1 – 3 , are the most powerful magnetic phenomena occurring on the Sun. Stars show magnetic activity…”
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  4. 4

    Chemical and physical processes caused by electrons impacting on H2O–CO mixed ices by Huang, C-H, Cecchi-Pestellini, C, Ciaravella, A, Jiménez-Escobar, A, Hsiao, L-C, Sie, N-E, Chen, Y-J

    “…ABSTRACT Electron-induced chemistry is relevant to many processes that occur when an ionizing source interacts with matter, as in the formation of complex…”
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    A systematic study of CO2 planetary atmospheres and their link to the stellar environment by Petralia, A, Alei, E, Aresu, G, Locci, D, Cecchi-Pestellini, C, Micela, G, Claudi, R, Ciaravella, A

    “…ABSTRACT The Milky Way Galaxy is literally teeming with exoplanets; thousands of planets have been discovered, with thousands more planet candidates…”
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    SOFT X-RAY IRRADIATION OF METHANOL ICE: FORMATION OF PRODUCTS AS A FUNCTION OF PHOTON ENERGY by Chen, Y-J, CIARAVELLA, A, CARO, G M MUNOZ, CECCHI-PESTELLINI, C, Jimenez-Escobar, A, Juang, K-J, Yih, T-S

    Published in The Astrophysical journal (01-12-2013)
    “…Pure methanol ices have been irradiated with monochromatic soft X-rays of 300 and 550eV close to the 1s resonance edges of C and O, respectively, and with a…”
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    X-Ray Photo-desorption of H2O:CO:NH3 Circumstellar Ice Analogs: Gas-phase Enrichment by Jiménez-Escobar, A., Ciaravella, A., Cecchi-Pestellini, C., Huang, C.-H., Sie, N.-E., Chen, Y.-J., Muñoz Caro, G. M.

    Published in The Astrophysical journal (20-11-2018)
    “…We study the photo-desorption occurring in H2O:CO:NH3 ice mixtures irradiated with monochromatic (550 and 900 eV) and broadband (250-1250 eV) soft X-rays…”
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  8. 8

    SOFT X-RAY IRRADIATION OF SILICATES: IMPLICATIONS FOR DUST EVOLUTION IN PROTOPLANETARY DISKS by Ciaravella, A., Cecchi-Pestellini, C., Chen, Y.-J., Muñoz Caro, G. M., Huang, C.-H., Jiménez-Escobar, A., Venezia, A. M.

    Published in The Astrophysical journal (01-09-2016)
    “…ABSTRACT The processing of energetic photons on bare silicate grains was simulated experimentally on silicate films submitted to soft X-rays of energies up to…”
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    BRIGHT RAY-LIKE FEATURES IN THE AFTERMATH OF CORONAL MASS EJECTIONS: WHITE LIGHT VERSUS ULTRAVIOLET SPECTRA by CIARAVELLA, A, Webb, D F, Giordano, S, Raymond, J C

    Published in The Astrophysical journal (20-03-2013)
    “…Current sheets (CSs) are important signatures of magnetic reconnection in the eruption of confined solar magnetic structures. Models of coronal mass ejections…”
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  10. 10

    Chemical Evolution of Interstellar Methanol Ice Analogs upon Ultraviolet Irradiation: The Role of the Substrate by Ciaravella, A., Jiménez-Escobar, A., Cosentino, G., Cecchi-Pestellini, C., Peres, G., Candia, R., Collura, A., Barbera, M., Cicca, G. Di, Varisco, S., Venezia, A. M.

    Published in The Astrophysical journal (01-05-2018)
    “…An important issue in the chemistry of interstellar ices is the role of dust materials. In this work, we study the effect of an amorphous water-rich magnesium…”
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  11. 11

    Effects of 150-1000 eV Electron Impacts on Pure Carbon Monoxide Ices Using the Interstellar Energetic-Process System (IEPS) by Huang, C.-H., Ciaravella, A., Cecchi-Pestellini, C., Jiménez-Escobar, A., Hsiao, L.-C., Huang, C.-C., Chen, P.-C., Sie, N.-E., Chen, Y.-J.

    Published in The Astrophysical journal (20-01-2020)
    “…Pure CO ice has been irradiated with electrons of energy in the range 150−1000 eV with the Interstellar Energetic-Process System. The main products of…”
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    UVCS/SOHO catalog of coronal mass ejections from 1996 to 2005: Spectroscopic proprieties by Giordano, S., Ciaravella, A., Raymond, J.C., Ko, Y.-K., Suleiman, R.

    “…Ultraviolet spectra of the extended solar corona have been routinely obtained by SOHO/UltraViolet Coronagraph Spectrometer (UVCS) since 1996. Sudden variations…”
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  13. 13

    CHEMICAL EVOLUTION OF A CO ICE INDUCED BY SOFT X-RAYS by Ciaravella, A., Chen, Y.-J., Cecchi-Pestellini, C., Jiménez-Escobar, A., Muñoz Caro, G. M., Chuang, K.-J., Huang, C.-H.

    Published in The Astrophysical journal (01-03-2016)
    “…ABSTRACT We irradiated a pure carbon monoxide ice with soft X-rays of energies up to 1.2 keV. The experiments were performed using the spherical grating…”
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    Ultraviolet Properties of Halo Coronal Mass Ejections: Doppler Shifts, Angles, Shocks, and Bulk Morphology by Ciaravella, A, Raymond, J. C, Kahler, S. W

    Published in The Astrophysical journal (20-11-2006)
    “…We present UV spectral information for 22 halo or partial halo CMEs observed by UVCS. The CME fronts show broad line profiles, while the line intensities are…”
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    Transition Region Emission from Solar Flares during the Impulsive Phase by Johnson, H, Raymond, J. C, Murphy, N. A, Giordano, S, Ko, Y.-K, Ciaravella, A, Suleiman, R

    Published in The Astrophysical journal (10-07-2011)
    “…There are relatively few observations of UV emission during the impulsive phases of solar flares, so the nature of that emission is poorly known. Photons…”
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