Noctilucent clouds are the highest clouds in the Earth’s atmosphere, 83 km (50 miles) and are observed slightly below the mesopause in the polar summertime. These clouds are of special interest, as they are sensitive to both global climate change and to solar/terrestrial influences. The first recorded sightings of noctilucent clouds were reported in 1885 and both satellite and ground-based observations over the past four decades have indicated that the presence of these clouds has been increasing in both frequency and brightness. Scientists now realize that these clouds are very sensitive indicators for what is going on in the atmosphere at higher altitudes as small changes in the atmospheric environment can lead to large changes in the properties of these clouds. Further, since these clouds form on condensation nuclei through cold temperatures and the presence of water vapor – and these properties of the mesosphere are tied to carbon dioxide and methane, the anthropogenic causes of climatic change may be directly related to the presence of noctilucent clouds.
Time lapse ground imagery of noctilucent clouds over Germany (credit: Gerd Baumgarten)
Noctilucent clouds are of significant interest within the aeronomy and climate science communities as noctilucent clouds are very sensitive indicators for what is going on in the atmosphere at higher altitudes. The extreme cold temperatures and very low density of the mesosphere creates an environment where very small changes in the atmosphere can drive large changes in observed noctilucent cloud properties. So by observing noctilucent clouds, we can learn a lot about the atmosphere as a whole (e.g. dynamical and thermal state, solar-terrestrial influences).
Since first observed in 1885, both satellite and ground observations throughout the last 40 years have indicated that 1) noctilucent clouds have increased in brightness over recent decades, 2) noctilucent clouds have extended to lower latitudes over recent decades, and 3) noctilucent clouds have been observed with increasing frequency over recent decades. What does this mean?
In general, clouds need two things to form: 1) low temperatures relative to the dew point, and 2) water vapor. We know that carbon dioxide acts as a net cooling agent in the upper atmosphere (though it warms the lower atmosphere, it radiates more heat away than it traps in the upper atmosphere, causing it to cool). Further, we know that methane photo-disassociates in the upper atmosphere and a major by-product is water vapor. Further, the introduction of chlorofluorocarbons (CFCs) in the lower atmosphere depletes the ozone, causing the stratosphere to shrink, and driving the mesosphere to be colder. As carbon dioxide, methane, and CFCs are all largely industrial by-products, they are believed to be man-made contributors to global climate change. So if we see more noctilucent clouds, colder temperatures and/or increased concentrations of water vapor must exist in the mesosphere, which may be caused by the introduction and upward convection of carbon dioxide, methane, and CFCs in the lower atmosphere.
Noctilucent clouds reside near a poorly understood yet critical region to reentry vehicles. The ground-track of space vehicles traveling to the International Space Station (ISS) missions reach latitudes where the low-latitude noctilucent clouds may be present. Since we don’t know enough about the mesosphere, manned space missions have chosen to act conservatively, enacting constraints for manned space missions that may be irrelevant. Through a better understanding of noctilucent clouds and the mesosphere, we may be able to design more operable space architecture.
By studying noctilucent clouds here on Earth, we can better model high-altitude, low-density clouds that may appear elsewhere, such as Mars!
Noctilucent clouds have been observed from the ground, through use of sounding rockets, from aircraft, and from a variety of spacecraft. The advent of reusable suborbital vehicles creates a radically new opportunity to study noctilucent clouds in ways that have either been impossible or cost prohibitive.
Noctilucent cloud ground observations have been recorded since 1885 and are visible from a specific latitudinal zone of approximately 50-65°. In visible wavelengths, noctilucent clouds scatter light more efficiently in the forward-scattering direction, which is the direction most germane to synchronous imagery with ground-based images. Ground imagery of noctilucent clouds have been consistently performed and cataloged from northward-observing ground sites since their initial observations, and it has been determined through repeated ground observations that noctilucent clouds are visible from range of Solar Depression Angle (SDA) from 6 to 16 degrees [Gadsden and Schroder, 1989]. Light Detection and Ranging (LiDAR) systems have more recently verified the altitudes and some vertical structure of noctilucent clouds, but they provide only point observations with limited time resolution and background removal.
Sounding rockets have provided in-situ observations and measurements of atmospheric constituents since 1962, when particle collectors revealed an abundance of particles of much greater size when the rocket penetrated a noctilucent cloud layer [Hemenway et al., 1964]. Later in 1982, the Cold Arctic Mesopause Project (CAMP) successfully mapped the temperature distribution of the summer mesopause [Philbrick et al., 1984]. Then in 1993, The NLC-93 rocket campaign at Esrange, Sweden, investigated the vertical structure of a noctilucent cloud layer in-situ, showing little vertical variation [Gumbel and Witt, 1998]. The question of particle size was further addressed in 1999 with the MIDAS-DROPPS rocket campaign, which used the scattering phase functions of NLCs through optical photometers [Gumbel et al., 2001]. Then in 2007, the PHOCUS rocket-borne experiment found no general difference between neutral and charged particles. [Hedin et al, 2007].
Satellite observations over nearly three decades have provided a consistent measure of polar mesospheric cloud occurrence, latitudinal extent, and brightness and indicate that the presence of these clouds has been increasing in frequency and extending to lower latitudes [Shettle et al., 2009;Deland et al., 2006]. American and Soviet astronauts have observed the phenomenon from space as early as 1970 and subsequent observations have been made from spaceborne platforms such as the Halogen Occultation Experiment (HALOE) and the Student Nitric Oxide Explorer (SNOE) [Merkel et al, 2003]. The most comprehensive advances to the understanding of polar mesospheric clouds have come from spaceborne platforms such as the Orbiting Geophysical Observatory (OGO-6), the Solar Mesospheric Explorer (SME), and most recently the AIM satellite.
The Aeronomy of Ice in the Mesosphere (AIM) Satellite is the first satellite with a primary mission dedicated to the study of polar mesospheric clouds. It has aboard it three payloads: 1) the Cloud Imaging and Particle Size (CIPS) instrument, providing a 2-D panoramic look at polar mesospheric clouds by collecting 360 degrees of multiple images, 2) the Solar Occultation for Ice Experiment (SOFIE) payload, measuring the variability of cloud particles with respect to their altitude and their chemical composition, and 3) the Cosmic Dust Explorer (CDE), recording the amount of space dust entering Earth’s atmosphere in order to assess whether space dust provides the foundation for the cloud condensation nuclei in the formation of noctilucent clouds. As shown in the image on the left, the AIM satellite typically makes fifteen overpasses each day. This plot shows how each overpass can be superimposed during a period of one day.
The advent of reusable suborbital vehicles provide a new capability to access this region of our atmosphere. Since the vehicle is reused, the costs of a suborbital flight to this region of our atmosphere and back are roughly ten times less than those of a comparable sounding rocket. And payloads can be placed on stabilized platforms and tended to by a human operator.
PoSSUM is designed to study these clouds using new balloon technologies and suborbital spacecraft through means never before available. Specifically, PoSSUM Scientist-Astronauts will construct 3D tomography of the microfeatures of these clouds, much like an MRI makes a 3D model of a person. This will reveal much about the dynamics and thermodynamics of the most sensitive region of our planet, the upper-atmosphere!
If we truly want to understand our climate and its changes, we need to understand our atmosphere. And to best understand our atmosphere as a whole, we need to understand the upper atmosphere, for this is the region where our planet interacts with our sun and the space environment. As such, both fluctuations in solar activity and small changes in our lower atmosphere, such as those created by man-made activities, will create large changes of observable phenomena in the upper atmosphere. With balloons, reusable suborbital vehicles, and PoSSUM’s remote sensing techniques, the opportunity now exists to study our climate and its changes in ways previously unavailable. PoSSUM has been formed to realize this opportunity.