Mukai, T.; Mukai, S.; Kikouchi, S. Variation of Grain Properties and the Dust Outbursts. Symposium on the Diversity and Similarity of Comets, ESA SP-278. European Space Agency. 1987: 427–30.
Grun, E.; Massonne; Schwehm, G. New Properties of Cometary Dust. Symposium on the Diversity and Similarity of Comets, ESA SP-278. European Space Agency. 1987: 305–14.
Simpson, J.; Rabinowitz, D.; Tuzzolino, A.; Ksanfomality, L. Halley's comet dust particle mass spectra, flux distributions and jet structures derived from measurements on the Vega-1 and Vega-2 spacecraft. ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 2: Dust and Nucleus. European Space Agency. 1986: 11–16.
Reach, W.; Sykes, M.; Kelley, M. Large Particles From Short-Period Comets. Workshop on Cometary Dust in Astrophysics. Houston: Lunar and Planetary Institute. 2003.
Kelley, M.; Reach, W.; Woodward, C. A Search for Deep Impact’s Large Particle Ejecta. Deep Impact as a World Observatory Event: Synergies in Space, Time, and Wavelength. Berlin Heidelberg: Springer-Verlag. 2009: 125. ISBN 978-3-540-76959-0.
Beech, M; Steel, D. On the definition of the term 'meteoroid'. Q. J. R. Astron. Soc. 1995, 36: 281–84. Bibcode:1995QJRAS..36..281B. Sec. 4 Lower size limit: Meteoroid or dust?
Rubin, A; Grossman, J. Meteorite and meteoroid: New comprehensive definitions. Meteoritics & Planetary Science. Mar 2010, 45 (1): 114–22. Bibcode:2010M&PS...45..114R. doi:10.1111/j.1945-5100.2009.01009.x. "...in practice the term is most often applied to objects smaller than approximately 100 um. These size ranges need to be modified." "By this definition, IDPs are particles smaller than 10um.""
Greenberg, M; Li, A. Morphological structural and chemical composition of cometary nuclei and dust. Space Science Reviews. 1997, 90: 149–61. S2CID 189789755. doi:10.1023/A:1005298014670. "tenth micron particles" "very fluffy aggregates"
Klöck, W; Staderman, F. Mineralogical and chemical relationships of interplanetary dust particles, micrometeorites, and meteorites in. LPI Technical Report 94-02 Workshop on the analysis of interplanetary dust particles. 1994. "50 um"
Levasseur-regourd, A; mukai; lasue; okada. physical properties of comet and interplanetary dust. Planetary and Space Science. 2007, 55 (9): 1010–20. Bibcode:2007P&SS...55.1010L. doi:10.1016/j.pss.2006.11.014. "a radius of 20 um for the upper cut-off"
Levasseur-Regourd, A; Mukai, T; Lasue, J; Okada, Y. Physical properties of comet and interplanetary dust. Planetary and Space Science. Jun 2007, 55 (9): 1010–20. Bibcode:2007P&SS...55.1010L. doi:10.1016/j.pss.2006.11.014. "20 um for the upper cut-off" "50 um for the upper cut-off"
Bradley, J; Sandford, S; Walker, R. 11.1 Interplanetary Dust Particles. Meteorites and the Early Solar System. University of Arizona Press. 1988: 861. "~ 10 um i diamtr" "~ 10-3 cm in dia"
Coulson, D; Wickramasinghe, N. Frictional and radiation heating of micron-sized meteoroids in the Earth's upper atmosphere. Mon. Not. R. Astron. Soc. 21 Aug 2003, 343 (4): 1123–30. Bibcode:2003MNRAS.343.1123C. doi:10.1046/j.1365-8711.2003.06478.x. "~10 um"
Folco, L; Cordier, C. 9. Micrometeorites. EMU Notes in Mineralogy. 2015. "10 um (Rubin and Grossman, 2010)""in the <100 um size fraction, i.e. across the transition between micrometeorites and IDPs"
Rietmeijer, F. Mesospheric Metal abundances and Meteoric Dust: Analysis of surviving Meteoroids. 34th COSPAR Scientific Assembly/2nd World Space Congress (196). Oct 2002. "stratospheric interplanetary dust particles (IDPs) (2-100 microns)" "debris from progenitors ~30 to ~1,000 microns"
Greenberg, J. From dust to comets. Comets, asteroids, meteorites: Interrelations, evolution and origins, Proceedings of the Thirty-Ninth International Colloquium. University of Toledo. 1977: 491.