Microwave Limb Sounder (MLS) experiments measure naturally-occurring microwave thermal emission from the limb (edge) of Earth's atmosphere to remotely sense vertical profiles of atmospheric gases, temperature, pressure, and cloud ice. The overall objective of these experiments is to provide information that will help improve our understanding of Earth's atmosphere and global change.

Aura MLS Data

Version 6 Data Release

The Aura Microwave Limb Sounder (MLS) team is pleased to announce the release of a new "version 6" (v6) MLS dataset. The most significant changes between v6 and the previous v5 data record are in the nitrous oxide (N2O) and temperature products. Although changes for other products are minimal, the MLS team recommends employing v6 in all new scientific studies using MLS data.

The v6 N2O product shows significantly larger abundances (by up to 20%) in the lower stratosphere (100-10 hPa) than v5, especially in the tropics, improving agreement with expectations and other observations. The v6 MLS temperature product has significantly better precision (up to 20% improvement) and vertical resolution (up to 30% improvement) in the upper stratosphere and lower mesosphere (10-0.1 hPa) compared to v5 and prior versions.

The entire Aura MLS data record since the July 2004 Aura launch to date has already been reprocessed using the v6 data processing software. The v6 software is also being used for forward processing of incoming MLS observations. To avoid disrupting scientific studies already well underway, forward processing of incoming MLS data using the previous v5 software will continue for the foreseeable future. In keeping with NASA ESDIS policy, with the release of MLS v6, the MLS v4 data record will no longer be available from the GES-DISC.

A full assessment of the MLS v6 data quality, along with guidelines for appropriate use of the data, is given in the data quality document. Importantly, this document describes updates to data screening rules for multiple products in v6. Of particular note is the limited remaining life of the MLS 190-GHz subsystem, which measures H2O, N2O, HCN, and upper stratospheric HNO3. Since May 2024, the 190-GHz measurements are only made for a few days each calendar month. The spectral regions MLS uses to measure several other species (notably CH3Cl, CH3CN, ClO, HCl, and cloud ice) are also affected by emission from water vapor. During periods when the 190-GHz subsystem is deactivated, in the absence of MLS H2O measurements, retrievals of those other species must assume climatological water vapor abundances. This introduces biases in those species such that, although they are still useful from a purely morphological or qualitative perspective, observations on affected days cannot be quantitatively compared to measurements taken on surrounding days or in previous years when the 190-GHz radiometer was operational. This issue applies equally to the MLS v5 data record (again, for observations starting in May 2024) and users of v5 data are advised to consult the v6 document for more information on this issue.

UPDATED - MLS "190 GHz" Observations Status

The MLS science team plans to "duty cycle" the 190-GHz observations (specifically of H2O, N2O, HCN, and upper stratospheric HNO3) to conserve remaining life for these measurements. The plan going forward is to reactivate the MLS 190-GHz subsystem for around six days each calendar month (plus a partial day for turn on and another for shutdown). As noted previously, depending on how the aging of the 190-GHz receiver progresses, we may lengthen or shorten each activation period by one or two days, but our aim will be to always have these measurements active around the middle of each calendar month. Substantial changes to this plan will be noted in future announcements.

The first of the reactivation periods (May 13-20, 2024) proceeded without issue, and we are on track to reactivate again on June 11, 2024, per the current duty cycle schedule.

In addition to H2O, N2O, HCN, and, for pressures less than 20 hPa, HNO3, which are not measured when the 190-GHz system is off, the MLS cloud products (Ice Water Content, IWC, and Ice Water Path, IWP) are also impacted and should not be used. Unfortunately, the effects on the IWC and IWP products are not properly flagged in the Level 2 data files, an issue that will be addressed in future versions of the MLS dataset.

Finally, note that MLS observations of other species (e.g., O3, HCl, ClO, CO, etc.) are unaffected by this issue.

Recent Publications

  1. Serva, F., L.D. Liberto, F. Colao, A. Bracci, F. Cairo, M. Pitts, and M. Snels, "Impact of the Hunga eruption on polar stratospheric clouds as seen by the lidar observatory at Concordia Station," Antarctic Science, 1-7, doi:10.1017/s0954102026100601, 2026.
  2. Zhou, X., Q. Chen, W. Feng, S. Heddell, S. Dhomse, G. Mann, H. Pumphrey, L. Millan, M. Santee, and M. Chipperfield, "Residence time of Hunga stratospheric water vapour perturbation quantified at 9 years," Nature Communications, Earth & Environment 7, 1, doi:10.1038/s43247-026-03216-5, 2026.