Hessdalen lights

The Hessdalen lights are unexplained nocturnal lights observed in a 7.5-mile-long (12 km) Hessdalen valley in rural central Norway.[1]

History and description

The Hessdalen lights are of unknown origin. They appear at night, and seem to float through and above the valley. They are usually bright white, yellow, or red and can appear above and below the horizon. The duration of the phenomenon may be from a few seconds to longer than an hour. Sometimes the lights move with enormous speed, while at other times they seem to sway slowly back and forth. On yet other occasions, they hover in mid‑air. Some hypothesise that the light is ionised iron dust.

Unusual lights have been reported in the region since at least the 1930s.[2] Especially high activity occurred between December 1981 and mid-1984, at which point the lights were being observed 15–20 times per week, which attracted many overnight tourists.[3] As of 2010, the lights were observed 10–20 times per year.

Research

Since 1983, there has been ongoing scientific research often nicknamed "Project Hessdalen", initiated by UFO-Norge and UFO-Sweden. The project was active as field investigations during 1983–1985. A group of students, engineers, and journalists collaborated as "The Triangle Project" in 1997–1998 and recorded the lights in a pyramid shape that bounced up and down.[4][5] In 1998, the Hessdalen Automatic Measurement Station (Hessdalen AMS) was built in the valley and registers and records the appearance of lights.

Later, the EMBLA programme was initiated. It brings together established scientists and students into researching these lights. Leading research institutions are Østfold University College (Norway) and the Italian National Research Council.

Hypotheses

Despite the ongoing research, there is no convincing explanation for the phenomenon. However, there are numerous working hypotheses.

  • Another hypothesis explains HL as a product of piezoelectricity generated under specific rock strains (Takaki and Ikeya, 1998)[8] because many crystal rocks include quartz grains which produce an intense charge density. In a 2011 paper,[11] based on the dusty plasma theory of HL, it is suggested that piezoelectricity of quartz cannot explain a peculiar property assumed by the HL phenomenon  the presence of geometrical structures in its center. Paiva and Taft have shown a mechanism of light ball cluster formation in Hessdalen lights by the nonlinear interaction of ion-acoustic and dusty-acoustic waves with low frequency geoelectromagnetic waves in dusty plasmas. The theoretical model shows that the velocity of ejected light balls by HL cluster is about 10,000 m s−1 in a good agreement with the observed velocity of some ejected light balls, which is estimated as 20,000 m s−1.[12] Why is the ejected ball always green-colored? Ejection of small green light ball from HL is due to radiation pressure produced by the interaction between very low frequency electromagnetic waves (VLF) and atmospheric ions (present in the central white-colored ball) through ion-acoustic waves (IAW).[13] Probably only O+
    2
    ions (electronic transition b4Σ
    g
    → a4Πu), with green emission lines, are transported by IAW. Electronic bands of O+
    2
    ions occur in auroral spectra.[14] Electron-molecular ion dissociative recombination coefficient rates α as functions of electron temperature Te, and cross sections σ as a function of electron energy E, have been measured by Mehr and Biondi[15] for N+
    2
    and O+
    2
    over the electron temperature interval 0.007–10 eV. The estimated temperature of HL is about 5,000 K.[9] In this temperature, the rate coefficients of dissociative recombination will be respectively α(Te)[O+
    2
    ] ~ 10−8 cm3 s−1, and α(Te)[N+
    2
    ] ~ 10−7 cm3 s−1. Thus, the nitrogen ions will be decomposed in N+
    2
    + e → N + N* more rapidly than oxygen ions in the HL plasma. Only ionic species are transported by IAW. Therefore, only oxygen ions will be predominant ejected green light balls from a central white ball in HL, presenting negative band of O+
    2
    with electronic transition b4Σ
    g
    → a4Πu after an IAW formation. Paiva and Taft presented a model for resolving the apparently contradictory spectrum observed in HL phenomenon. Thus, its nearly flat spectrum on the top with steep sides is due to the effect of optical thickness on the bremsstrahlung spectrum. At low frequencies self-absorption[16] modifies the spectrum to follow the Rayleigh–Jeans part of the blackbody curve. This spectrum is typical of dense ionized gas. Additionally, the spectrum produced in the thermal bremsstrahlung process is flat up to a cutoff frequency, νcut, and falls off exponentially at higher frequencies. This sequence of events forms the typical spectrum of HL phenomenon when the atmosphere is clear, with no fog. According to the model, spatial color distribution of luminous balls commonly observed in HL phenomenon are produced by electrons accelerated by electric fields during rapid fracture of piezoelectric rocks under the ground.[17]

See also

References

  1. 1 2 Leone, Matteo (2003). "A rebuttal of the EMBLA 2002 report on the optical survey in Hessdalen" (PDF). Comitato Italiano per il Progetto Hessdalen. pp. 1–29. Archived (PDF) from the original on 2014-02-07.
  2. Zanotti, Ferruccio; Di Giuseppe, Massimiliano; Serra, Romano. "Hessdalen 2003: Luci Misteriose in Norvegia" (PDF) (in Italian). Comitato Italiano per il Progetto Hessdalen. pp. 4–5. Archived (PDF) from the original on 2016-01-04.
  3. Pāvils, Gatis (2010-10-10). "Hessdalen lights". Wondermondo. Archived from the original on 2015-07-02.
  4. Ballester Olmos, Vicente‑Juan; Brænne, Ole Jonny (2008). "11 October 1997". Norway in UFO Photographs: The First Catalogue. FOTOCAT. 4. Torino: UPIAR. p. 94. LCCN 2010388262. OCLC 713018022. Archived (PDF) from the original on 2015-12-29.
  5. Olsen, Andreas, ed. (1998). "The Triangle Project". Archived from the original on 2002-10-17.
  6. Johansen, Karl Hans (2007-07-16). "Fenomenet Hessdalen" (in Norwegian). Norsk rikskringkasting. Archived from the original on 2015-07-03.
  7. Hauge, Bjørn Gitle (2007). Optical spectrum analysis of the Hessdalen phenomenon (PDF) (Report). Archived (PDF) from the original on 2014-08-30.
  8. 1 2 Paiva, Gerson S.; Taft, Carlton A. (2010). "A hypothetical dusty plasma mechanism of Hessdalen lights". Journal of Atmospheric and Solar-Terrestrial Physics. 72 (16): 1200–1203. doi:10.1016/j.jastp.2010.07.022. ISSN 1364-6826. OCLC 5902956691. (subscription required (help)).
  9. 1 2 Teodorani, Massimo (2004). "A Long-Term Scientific Survey of the Hessdalen Phenomenon" (PDF). Journal of Scientific Exploration. Petaluma, California. 18 (2): 217–251. ISSN 0892-3310. Archived (PDF) from the original on 2015-12-28.
  10. Johnston, Hamish (2007-08-15). "Helices swirl in space-dust simulations". Physics World. Archived from the original on 2015-12-28.
  11. Paiva, Gerson S.; Taft, Carlton A. (2011). "Hessdalen Lights and Piezoelectricity from Rock Strain" (PDF). Journal of Scientific Exploration. Petaluma, California: Society for Scientific Exploration. 25 (2): 265–271. ISSN 0892-3310. OCLC 761916772. Archived from the original (PDF) on 2015-12-28.
  12. Paiva, Gerson S.; Taft, Carlton A. (2012). "Cluster formation in Hessdalen lights". Journal of Atmospheric and Solar‑Terrestrial Physics. 80: 336–339. doi:10.1016/j.jastp.2012.02.020. ISSN 1364-6826. OCLC 4934033386. (subscription required (help)).
  13. Paiva, Gerson S.; Taft, Carlton A. (2011). "Color Distribution of Light Balls in Hessdalen Lights Phenomenon". Journal of Scientific Exploration. 25 (4): 735–746. ISSN 0892-3310.
  14. Chamberlain, J.W., Physics of the Aurora and Air-glow (Academic Press Inc. , New York, 1961)
  15. Mehr, F J; Biondi, M A (1969). "Electron temperature dependence of recombination O+
    2
    and N+
    2
    ions with electrons". Phys. Rev. 181: 264–271.
  16. Paiva, Gerson S.; Taft, Carlton A. (2012). "A mechanism to explain the spectrum of Hessdalen Lights phenomenon". Meteorology and Atmospheric Physics. 117 (1–2): 1–4. doi:10.1007/s00703-012-0197-5.
  17. Paiva, Gerson S.; Taft, C. A (2011). "Color Distribution of Light Balls in Hessdalen Lights Phenomenon". J. Sc. Expl. 25: 735.

External links

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