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Juno Jupiter image

Namrah Habib

Postdoctoral Research Assistant in Space Instrumentation

Research theme

  • Astronomy and astrophysics
  • Instrumentation
  • Exoplanets and planetary physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Exoplanet atmospheres
  • Exoplanets and Stellar Physics
  • Planetary Climate Dynamics
  • Planetary surfaces
  • Solar system
  • Space instrumentation
  • About
  • Publications

The Lunar Trailblazer Lunar Thermal Mapper Instrument

(2025)

Authors:

Neil E Bowles, Bethany L Ehlmann, Rory Evans, Tristram Warren, Henry Hall Eshbaugh, Greg King, Waqas Mir, Namrah Habib, Katherine A Shirley, Fraser Clarke, Cyril Bourgenot, Chris Howe, Keith Nowicki, Fiona Henderson, Christopher Scott Edwards, Rachel Louise Pillar Klima, Kerri L Donaldson Hanna, Calina Seybold, Andrew Klesh, David Ray Thompson, Elise Furlan, Elena Scire, Judy Adler, Nicholas Elkington, Aria Vitkova, Jon Temple, Simon Woodward
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3D Modeling of Moist Convective Inhibition in Hydrogen-Dominated Atmospheres

(2024)

Authors:

Namrah Habib, Raymond T Pierrehumbert
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Modeling Noncondensing Compositional Convection for Applications to Super-Earth and Sub-Neptune Atmospheres

The Astrophysical Journal American Astronomical Society 961:1 (2024) 35-35

Authors:

Namrah Habib, Raymond T Pierrehumbert

Abstract:

Abstract Compositional convection is atmospheric mixing driven by density variations caused by compositional gradients. Previous studies have suggested that compositional gradients of atmospheric trace species within planetary atmospheres can impact convection and the final atmospheric temperature profile. In this work, we employ 3D convection-resolving simulations using Cloud Model 1 (CM1) to gain a fundamental understanding of how compositional variation influences convection and the final atmospheric state of exoplanet atmospheres. We perform 3D initial value problem simulations of noncondensing compositional convection for Earth-air, H 2 , and CO 2 atmospheres. Conventionally, atmospheric convection is assumed to mix the atmosphere to a final, marginally stable state defined by a unique temperature profile. However, when there is compositional variation within an atmosphere, a continuous family of stable end states is possible, differing in the final state composition profile. Our CM1 simulations are used to determine which of the family of possible compositional end states is selected. Leveraging the results from our CM1 simulations, we develop a dry convective adjustment scheme for use in general circulation models (GCMs). This scheme relies on an energy analysis to determine the final adjusted atmospheric state. Our convection scheme produces results that agree with our CM1 simulations and can easily be implemented in GCMs to improve modeling of compositional convection in exoplanet atmospheres.
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Details from ORA
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Modelling Non-Condensing Compositional Convection for Applications to Super-Earth and Sub-Neptune Atmospheres

(2023)

Authors:

Namrah Habib, Raymond T Pierrehumbert
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Geophysical constraints on the properties of a subglacial lake in northwest Greenland

The Cryosphere Copernicus GmbH 15:7 (2021) 3279-3291

Authors:

Ross Maguire, Nicholas Schmerr, Erin Pettit, Kiya Riverman, Christyna Gardner, Daniella N DellaGiustina, Brad Avenson, Natalie Wagner, Angela G Marusiak, Namrah Habib, Juliette I Broadbeck, Veronica J Bray, Samuel H Bailey

Abstract:

Abstract. In this study, we report the results of an active-source seismology and ground-penetrating radar survey performed in northwestern Greenland at a site where the presence of a subglacial lake beneath the accumulation area has previously been proposed. Both seismic and radar results show a flat reflector approximately 830–845 m below the surface, with a seismic reflection coefficient of −0.43 ± 0.17, which is consistent with the acoustic impedance contrast between a layer of water and glacial ice. Additionally, in the seismic data we observe an intermittent lake bottom reflection arriving between 14–20 ms after the lake top reflection, corresponding to a lake depth of approximately 10–15 m. A strong coda following the lake top and lake bottom reflections is consistent with a package of lake bottom sediments although its thickness and material properties are uncertain. Finally, we use these results to conduct a first-order assessment of the lake origins using a one-dimensional thermal model and hydropotential modeling based on published surface and bed topography. Using these analyses, we narrow the lake origin hypotheses to either anomalously high geothermal flux or hypersalinity due to local ancient evaporite. Because the origins are still unclear, this site provides an intriguing opportunity for the first in situ sampling of a subglacial lake in Greenland, which could better constrain mechanisms of subglacial lake formation, evolution, and relative importance to glacial hydrology.
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