Search Results - "Ramelli, Renzo"

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  1. 1

    Reconstruction of the Sunspot Number Source Database and the 1947 Zurich Discontinuity by Clette, Frédéric, Lefèvre, Laure, Bechet, Sabrina, Ramelli, Renzo, Cagnotti, Marco

    Published in Solar physics (01-09-2021)
    “…The recalibration of the sunspot number series, the primary long-term record of the solar cycle, requires the recovery of the entire collection of raw sunspot…”
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    Journal Article
  2. 2

    Robotic and Non-Robotic Control of Astrophysical Instruments by Küveler, Gerd, Dao, Van Dung, Zuber, Axel, Ramelli, Renzo

    Published in Advances in astronomy (01-01-2010)
    “…We present a system of device control programs, developed for the solar observatory at Locarno/Switzerland (IRSOL). Because these programs are implemented as…”
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    Journal Article
  3. 3

    Sunspot Observations and Counting at Specola Solare Ticinese in Locarno Since 1957 by Cortesi, Sergio, Cagnotti, Marco, Bianda, Michele, Ramelli, Renzo, Manna, Andrea

    Published in Solar physics (01-11-2016)
    “…Specola Solare Ticinese is an observatory dedicated to sunspot number counting. It was constructed in 1957 in Locarno, Southern Switzerland, as an external…”
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    Journal Article
  4. 4

    Reconstruction of the Sunspot Number Source Database and the 1947 Zurich Discontinuity by Clette, Frédéric, Lefèvre, Laure, Bechet, Sabrina, Ramelli, Renzo, Cagnotti, Marco

    Published 06-01-2023
    “…Solar Physics, Volume 296, Issue 9, article id.137, 2021 The recalibration of the sunspot number series, the primary long-term record of the solar cycle,…”
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    Journal Article
  5. 5

    Hanle rotation signatures in Sr I 4607 {\AA} by Zeuner, Franziska, Belluzzi, Luca, Guerreiro, Nuno, Ramelli, Renzo, Bianda, Michele

    Published 06-05-2022
    “…A&A 662, A46 (2022) Observations of scattering polarization and the Hanle effect in various spectral lines are increasingly used to complement traditional…”
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    Journal Article
  6. 6

    Robotic and Non-Robotic Control of Astrophysical Instruments by Küveler, Gerd, Dao, Van Dung, Zuber, Axel, Ramelli, Renzo

    Published in Advances in astronomy (2010)
    “…We present a system of device control programs, developed for the solar observatory at Locarno/Switzerland (IRSOL). Because these programs are implemented as…”
    Get full text
    Journal Article
  7. 7

    Characterization of a thinned back illuminated MIMOSA V sensor as a visible light camera by Bulgheroni, Antonio, Bianda, Michele, Caccia, Massimo, Cappellini, Chiara, Mozzanica, Aldo, Ramelli, Renzo, Risigo, Fabio

    “…This paper reports the measurements that have been performed both in the Silicon Detector Laboratory at the University of Insubria (Como, Italy) and at the…”
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  8. 8

    Sunspot data collection of Specola Solare Ticinese in Locarno by Ramelli, Renzo, Cagnotti, Marco, Cortesi, Sergio, Bianda, Michele, Manna, Andrea

    Published 23-05-2018
    “…Sunspot observations and counting are carried out at the Specola Solare Ticinese in Locarno since 1957 when it was built as an external observing station of…”
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    Journal Article
  9. 9

    Measurement of the evolution of the magnetic field of the quiet photosphere during a solar cycle by Ramelli, Renzo, Bianda, Michele, Berdyugina, Svetlana, Belluzzi, Luca, Kleint, Lucia

    Published 10-08-2017
    “…The solar photosphere is filled by a magnetic field which is tangled on scales much smaller than the resolution capability of solar telescopes. This hidden…”
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    Journal Article
  10. 10

    Observations on spatial variations of the Sr~{\sc i} 4607~\AA~scattering polarization signals at different limb distances with ZIMPOL by Dhara, Sajal Kumar, Capozzi, Emilia, Gisler, Daniel, Bianda, Michele, Ramelli, Renzo, Berdyugina, Svetlana, Alsina, Ernest, Belluzzi, Luca

    Published 09-08-2019
    “…The Sr~{\sc i} 4607~\AA\ spectral line shows one of the strongest scattering polarization signals in the visible solar spectrum. The amplitude of this…”
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    Journal Article
  11. 11

    Spatial variations of the SrI 4607\AA scattering polarization signals at subgranular scale observed with ZIMPOL at GREGOR telescope by Dhara, Sajal Kumar, Capozzi, Emilia, Gisler, Daniel, Bianda, Michele, Ramelli, Renzo, Berdyugina, Svetlana, Alsina, Ernest, Belluzzi, Luca

    Published 08-04-2019
    “…Sr I 4607\AA spectral line shows one of the strongest scattering polarization signals in the visible solar spectrum. The amplitudes of these signals are…”
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    Journal Article
  12. 12

    Sunspot Observations and Counting at Specola Solare Ticinese in Locarno since 1957 by Cortesi, Sergio, Cagnotti, Marco, Bianda, Michele, Ramelli, Renzo, Manna, Andrea

    Published 25-02-2016
    “…Specola Solare Ticinese is an observatory dedicated to Sunspot Number counting, which was constructed in 1957 in Locarno, Southern Switzerland, as an external…”
    Get full text
    Journal Article
  13. 13

    Helium Emissions Observed in Ground-Based Spectra of Solar Prominences by Ramelli, Renzo, Stellmacher, Goetz, Wiehr, Eberhard, Bianda, Michele

    Published 02-10-2012
    “…2012SoPh..281..697W The only prominent line of singly ionized helium in the visible spectral range, helium-II 4686 A, is observed together with the helium-I…”
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  14. 14

    He-D3 Polarization observed in Prominences by Ramelli, Renzo, Bianda, Michele

    Published 23-01-2004
    “…Spectro-polarimetric measurements of the D3-HeI 5876 A line profile in 35 prominences have been performed in 2003 with the Gregory-Coud\'e Telescope in…”
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    Journal Article
  15. 15

    Scattering polarization and the Hanle effect in H-alpha as a probe of chromospheric magnetism: Modeling vs. Observations by Stepan, Jiri, Bueno, Javier Trujillo, Ramelli, Renzo, Bianda, Michele

    Published 24-02-2011
    “…The Hanle effect in strong spectral lines is the physical mechanism that should be increasingly exploited for quantitative explorations of the magnetism of the…”
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  16. 16

    The power spectrum of the seeing during solar observations by Sigismondi, Costantino, Raponi, Andrea, Wang, Xiaofan, De Rosi, Giulia, Bianda, Michele, Ramelli, Renzo

    Published 02-12-2011
    “…Measurements of the power spectrum of the atmospheric seeing in the line of sight of the Sun, in the range 0.001-1 Hz, have been performed in Santa Maria degli…”
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  17. 17

    Atmospheric fluctuations below 0.1 Hz during drift-scan solar diameter measurements by Sigismondi, Costantino, Raponi, Andrea, De Rosi, Giulia, Bianda, Michele, Ramelli, Renzo, Caccia, Massimo, Maspero, Matteo, Negrini, Loretta, Wang, Xiaofan

    Published 28-12-2011
    “…Measurements of the power spectrum of the seeing in the range 0.001-1 Hz have been performed in order to understand the criticity of the transits' method for…”
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