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Appendix I: List of Responses to Request for Information
Pages 412-440

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From page 412...
... TABLE I.1  Responses to Request for Information RFI Response Number First Author Response Title Summary Description 1 Ali, Nancy A., et al. Recommendations for Education/Public Addresses EPO as a major contributing factor Outreach (EPO)
From page 413...
... Improved Space Weather Situational Awareness 7 Bala, Ramkumar Space Weather Forecasting through Advocates for stronger community participation. Association 8 Balch, Christopher The Next Step in Heliospheric Proposes an enhanced interplanetary observing C
From page 414...
... characterization of the ionosphere using optical tomography. 22 Budzien, Scott A., Heterogeneous Measurements for Emphasizes that space weather forecasting with et al.
From page 415...
... Space Physics Observation Platform V2 Japanese Experiment Module is suitable for siting optical instrumentation and conducting scientific experiments. continued
From page 416...
... , surface magnetic fields, transition region, and extended corona from an orbit inclined at least 40 degrees to the ecliptic plane. 41 Clarke, John T., White Paper on Comparative Planetary Recommends the observation of planetary and et al.
From page 417...
... 51 Davila, Joseph M., The International Space Weather Details the deployment of 100 new instruments et al. Initiative (ISWI)
From page 418...
... 61 Dyrud, Lars, et al. A Crucial Space Weather Effect: Meteors Describes the importance of the interplanetary and Meteoroids meteoroid and dust environment to support studies of solar system evolution, solar wind, upper atmospheric physics, planetary atmospheres and ionospheres, planetary geology, and manned and unmanned spacecraft.
From page 419...
... 73 Fennell, J.F. Enhancement of POES Instruments to Encourages the National Oceanic and Provide Better Space Weather Electron Atmospheric Administration (NOAA)
From page 420...
... current space weather objectives with three paired constellations of small satellites flying in multiple orbits.
From page 421...
... 98 Goode, Philip The 1.6 m Clear Aperture Optical Solar Describes how the largest aperture (1.6 m) solar Telescope in Big Bear -- The NST telescope will provide an essential complement to SDO, Hinode, and other satellite data, especially as a probe of the space weather.
From page 422...
... 111 Huang, Cheryl A Satellite Mission Concept to Study Presents a satellite mission concept to study Thermosphere-Ionosphere Coupling ion-neutral coupling with an improvement in satellite drag modelling. 112 Huba, Joseph D., A Comprehensive, First-Principles Model Discusses the development of a new et al.
From page 423...
... 116 Israel, Martin H., The Effect of the Heliosphere on Recommends improving observations of galactic et al. Galactic and Anomalous Cosmic Rays cosmic rays and anomalous cosmic rays to better understand how the interplanetary magnetic field modulates both galactic and anomalous cosmic rays in the inner solar system.
From page 424...
... of Solar Magnetic Fields magnetic fields on their natural physical scales with a large-aperture solar telescope, namely ATST. 132 Keiling, Andreas Science and Mission Concept of a Outlines a holistic ground-spacecraft mission Holistic Ionosphere-Auroral Zone- with four-point conjunctions along magnetic Magnetosphere Investigation flux tubes connecting the ionosphere, the auroral acceleration region, and the outer magnetosphere.
From page 425...
... (CubeSats and Nanosatellites) in miniaturization, new manufacturing techniques, Support of Heliophysics Research and and new materials and the development of a the National Space Weather Program cadre of commercial suppliers of small satellite subsystems fortify the technical readiness of CubeSats for heliophysics research.
From page 426...
... Solar Wind and Suprathermal Ion Discusses the vital role of solar wind and Composition Measurements: An suprathermal composition measurements in Essential Element of Current and Future resolving major outstanding science questions Space Missions regarding reconnection, particle acceleration, and improving space weather predictions. 152 Lessard, Marc R., The Importance of Ground- Describes the importance of high-latitude et al.
From page 427...
... particles reaching at Earth, the loss rate of Earth's radiation belt electrons, and the effect of these energetic particles on the chemistry and dynamics of Earth's middle and upper atmosphere. 156 Liewer, Paulett C., Solar Polar Imager: Observing Solar Proposes a mission to target the unexplored et al.
From page 428...
... 170 Mabie, Justin J A Comprehensive and Continuous Recommends steps to modernize a Record of Ground Based Space Weather comprehensive climatology of ground-based Observations space weather observations collected from magnetometers, ionosondes, and other methods.
From page 429...
... Ground-based Space Weather Proposes that the geoscience community foster Instrument Suites a class of instrumentation that involves multi instrument, ground-based suites similar to satellite instrumentation. 180 Martinis, Carlos Neutral Winds in the Upper Atmosphere Discusses the need to measure neutral winds in the upper atmosphere in a global spatial and temporal scale to understand many processes involving electro-dynamics and ion-neutral coupling.
From page 430...
... 197 Mertens, Nowcast of Atmospheric Ionizing Describes the Nowcast of Atmospheric Ionizing Christopher J., et al. Radiation for Aviation Safety Radiation for Aviation Safety, a prototype operational model for predicting commercial aircraft radiation exposure from galactic and solar cosmic rays.
From page 431...
... Ionosphere Decoupling Investigations assumption of polar cap symmetry in ring current and radiation belt models. 204 Mlynczak, Martin Spectral Signatures of Geospace Proposes continued measurement of infrared G., et al.
From page 432...
... Research Funding U.S. civilian agencies for basic space physics research and the development of space weather applications, maintaining distinct requirements for both.
From page 433...
... 226 Retterer, John M Next Gen IT Modeling Infrastructure for Describes new infrastructure required for Space Weather Forecasting progress in ionosphere/thermosphere modeling, both for scientific progress and operational utility.
From page 434...
... 239 Schreiner, William Using Space-Based GNSS Radio Addresses the scientific and operational needs S Occultation Data for Ionospheric and for continuing global observations of the Space Weather Applications ionosphere and lower neutral atmosphere with Global Navigation Satellite System radio occultation data.
From page 435...
... , the Sun, in the Habitability of Its Planets, including understanding the solar magnetic and in Space Weather around Earth dynamo by combining numerical studies and theory with observations of the evolving surface field of Sun and stars and of solar and stellar internal flows. 241 Schwadron, N.A., Research to Operations (Res2Ops)
From page 436...
... irradiances should continue to be a priority of the heliophysics community for understanding both the long-term (climate) and short-term (space weather)
From page 437...
... Mapping Across necessary routine space weather maps of the Temporal and Spatial Scales near-Earth space weather volume for both scientific inquiry and operational users by combining global imaging and low-altitude sensors measuring ultraviolet airglow. 259 Stevens, Michael Direct Observations of Global-Scale Describes a mission to study global-scale H., et al.
From page 438...
... , a facility dedicated to the measurement of magnetic fields and plasma properties in the solar corona to advance understanding of the Sun's generation of space weather. 269 Tylka, Allan J
From page 439...
... . 278 White, Stephen M., Coronal Magnetic Fields Outlines the difficulties in making advances et al.
From page 440...
... 288 Zhu, Ping Meso Scale Transients in Magnetotail Proposes to systematically investigate meso and Their Roles in Substorm Dynamics scale transients in the magnetotail, which may play key roles in mediating and regulating the transition process from the late substorm growth phase to the beginning of onset expansion.


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